As you look over your new RCX telescope, one of the first things you will notice is that it has no Focus Knob!
Because this design is of key importance, we are presenting this information on how to focus your telescope on the inside
front cover so that it is immediately accessible.
The Focus Key
All focusing of the RCX400 is performed digitally, using AutoStar II’s Focus key (number key 4).
The Focus ke
J Press the Focus key the first time to focus the telescope and to control
the speed at which you focus.
J Press the Focus key again to set and adjust up to nine focus presets.
To change the focus speed:
1.Press the Focus key once. “Focuser: Fast (or the current speed)” displays for two seconds. Use one of the Scroll keys to
scroll through the list of 4 a
desire displays. Choose a focus speed with which you feel comfortable.
To focus the telescope:
1.Press the Focus key once. “Focuser: Fast (or the current speed)” displays. After two seconds, “Focuser: Position = XX” displays. “XX” stands for a number value in decimal millimeters.
2.Point the telescope at a distant object. Look in the eyepiece and use the Arrow keys until the image in the eyepiece is in
focus.
To exit the focus operation at any time:
1.Press MODE.
If you wish learn how to set focus presets, see page 19.
y functions as a toggle key:
vailable focus speeds: Fast, Medium, Slow, Fine. Scroll through the list until the speed you
How to Hot Swap the Autostar II Handbox
You may move the Autostar II handbox from one computer control panel to another, without turning off the RCX control panel.
This is called “hot swapping.”
o hot swap the handbox:
T
1.Unplug the handbox connector and plug Autostar II into the HBX port of the other computer control panel.
2.Press and hold the “?” key for two seconds to refresh the display.
WARNING!
Never use a Meade
look at the Sun! Looking at or near the Sun
will cause instant and irreversible damage to
your eye. Eye damage is often painless, so
there is no warning to the observer that damage has occurred until it is too late. Do not
point the telescope or its viewfinder at or
near the Sun. Do not look through the telescope or its viewfinder as it is moving.
Children should always have adult supervision while observing.
Caution: Use care to install batteries in the
orientation indicated by illustration in the battery slots of the battery holder. Follow battery
manufacturer's precautions. Do not install
batteries backwards or mix new and used
batteries. Do not mix battery types. If these
precautions are not followed, batteries may
explode, catch fire, or leak. Improperly
installed batteries void your Meade warranty.
® The name "Meade" and the Meade logo are trademarks
registered with the U.S. Patent Office and in principal countries throughout the world. "RCX400 " and "AutoStar II" are
ks of Meade Instruments Corporation.
ademar
tr
P
atents:
US 6,304,376
US 6,392,799
US 6,563,636
D 422,610
Patent Pending.
STEP 1: Attach the legs of the tripod to the base:
Slide each leg (1) into a leg receptacle (2) .
c
B
STEP 2: Rotate the leg:
Rotate the leg until the trigger release pin (3) is next to the
thruster bar latch (4).
f
g
A
f
d
e
e
d
B
STEP 3: “Hook” the Release Pin:
Slide thruster bar hook into the slot in the trigger release pin.1
Take note of the trigger release lever (5) on the base; you will use
the release lever in Step 5 below. The trigger release consists of
a lever on one side and a pin that runs through to the other side
of the base.
STEP 4: Tighten the adjustment lock:
Rotate the leg attachment lock (6) and tighten to a firm feel.
STEP 5: Set the height of your tripod:
Press and hold down (A) the trigger release lever (5) slide the tripod leg to the desired length (thereb
pod).
Important Step: Let go of the trigger (B) when the tripod leg
is at the desired length. Unhook the trigger release pin to
lock the leg in place. This step prevents your tripod accidentally slipping out of the position you set .
Perform this procedure for each of the tripod’s legs. The tripod
should now be stable.
y setting the height of the tr
i-
4
Attach the Mount to the Tripod
j
h
i
STEP 6: P
Take note of the T-handle/rod (8) that goes through the tripod
base. The T-handle/rod is spring-mounted into position. Note also
that there is a hole (7) on the bottom side of the mount base
Lift the mount and position the mount base over the tripod base.
Line up the hole on the mount base over the T-handle rod. When
they are lined up, the rod will “pop up” into the hole.
Caution for 12” and 14” model users: Due to the weight and
size of these products, please use extreme caution whenever
assembling, disassembling, lifting, transporting or storing these
products. Two or more persons should always be used whenever
performing any of these tasks. Disregard for the above warning
could result in serious injury or death.
STEP 7: Secure the mount with the T-handle:
Rotate the T-handle (9) until the rod is tightened to a firm feel.
osition the mount over the tripod:
.
Move the Optical Tube and Install the Batteries
STEP 8: Move the optical tube from its shipping position:
Turn the Dec. lock (10) counterclockwise to unlock the the optical
tube (11) and move it perpendicular the fork arms, to the position
depicted in the image at the left. Turn the Dec. lock clockwise to a
firm feel to relock the position of the optical tube.
1)
STEP 9: Install the batteries:
ly of the
ies. Remove the battery compartment (13) covers
e compar
RCX400 telescope requires eight C-cell (user
Retur
y holder
tments and replace the co
.
1!
Assemb
supplied) batter
and carefully remove the battery holders (12), being mindful of the
connector wires.
Insert four user-supplied C-cell batteries into each battery
holder, oriented as shown on the diagram on the battery slots
inside the batter
respectiv
1#
Caution: Use care to install batteries as indicated by the battery
compartment. Follow battery manufacturer's precautions. Do not
install batteries backwards or mix new and used batteries. Do not
mix battery types. If these precautions are not followed, batteries
1@
may explode, catch fire, or leak.
Improperly installed batteries void your Meade warranty. Always
ve the batteries if they are not to be used for a long period
remo
of time.
n the batter
y holders to their
vers.
5
QUICK-START GUIDE {CONTINUED}
Insert the Telescope Diagonal Mirror and Eyepiece
1%
1(
2)
1*
1&
1^
STEP 10: Attach the visual back and diagonal mirror:
1.Thread the ring of the visual back (16) over the rear cell (15)
and rotate the r
onal (18) into the visual back and secure it in place using
the visual back thumbscrew (17).
STEP 11: Insert the eyepiece and remove dust cover:
Remove the UltraWide 24mm eyepiece (19) from its
container and place it in the diagonal mirror. Tighten the thumbscrew (20) located on the diagonal mirror to a firm feel only.
Remove the dust cover (
tube assembly (
ing, tightening to a firm feel. Slide the diag-
18, Fig. 1a) from the front of the optical
19, Fig. 1a) by gently prying it off.
2#
2$
2%
2^
2!
2@
STEP 12: Plug in the AutoStar II handbox
Check that the power switch on the computer control panel (21)
is in the OFF position. Plug the coil cord of the AutoStar II handbox into the HBX port of the base control panel (22).
Note: The AutoStar II handbox does not require batteries; the
batteries in the telescope supply the power.
Note: You can only plug one handbox into the telescope at a
time; you cannot plug two handboxes into the two control panels
at the same time.
STEP 13: T
Press the Power Switch on the computer control panel to the ON
position. The copyright message lights on AutoStar II's LCD display (23).
Press the key prompted by AutoStar II to accept the Sun warning. AutoStar II now displays "Automatic Alignment." You can
then use the Arrow keys (24) to slew (move) the
telescope up, down, right, or left.To change the telescope’s slew
speed, press the Speed key (25) and then the Number keys (26).
"9" is the f
urn on AutoStar:
astest speed and "1" is the slo
est speed.
w
6
Point, Focus and Observe
2&
2(
STEP 14: Tighten the R.A. and Dec. Locks:
Move the R.A. lock (27) and tighten to a firm feel. Rotate the Dec.
Lock (28) and tighten to a firm feel, also.
2*
STEP 15: Focus:
To change the focus speed:
Press the Focus key (2() once. “Focuser: Fast (or the current
speed)” displays. Use one of the Scroll keys to scroll through the
list of 4 available focus speeds: Fast, Medium, Slow, Fine. Scroll
through the list until the speed you desire displays (choose a
focus speed with which you feel comfortable).
To focus the telescope:
1. Press the Focus key once. “Focuser: Fast (or the current
speed)” displays. After two seconds, “Focuser: Position = XX” displays. “XX” stands for a number value in decimal millimeters.
2. Point the telescope at a distant object. Look in the eyepiece
and press the Arrow keys until the image in the eyepiece is in
focus.
To exit the focus operation:
1. Press MODE.
STEP 16: Point and Observe:
Sight along the side of the telescope tube to locate an object (if
you wish to attach the viewfinder, see page 18 for more information).
Look through the eyepiece and use AutoStar’s arrow keys to center the object in your eyepiece.
WHERE
See pages 8 to 12 to learn about your tripod and telescope’s features.
See pages 13 to 15 to learn about AutoStar II’s features.
See pages 16 to 17 to learn more about your telescope’s
assemb
See page 18 to lear
See pages 19 to 21 to learn more about observing and
ocusing with your scope.
f
See pages 22 to 24 to lear
to” with your telescope.
See pages 28 to 44 to learn about AutoStar’s menus.
See pages 45 to 47 to lear
telescope
See pages 48 to 50 to learn about optional accessories
vailable for your scope.
a
TO GO FROM HERE...
.
ly
n about y
n ho
n about photog
.
our telescope’
w to initializ
wfinder
s vie
, align and
e
y and your
aph
r
.
“go
7
TELESCOPE FEATURES
B
c
d
e
eyepiece
diagonal
mirror
rear cell and
2” visual back
OTA control
panel
2!
viewfinder
2)
fan
1(
optical tube
dust cover
Dec. lock
Dec. slow
motion control
right fork arm
1*
1&
1^
1%
handles
f
left fork arm
g
battery
h
compartments
R.A. slow motion control
i
Base control panel
j
GPS
1)
Receiv
Dec Setting
Circle
1!
AutoStar II
handbox and
tiltable holder
R.A. lock
1$
1#
mounting base
1@
er
on the left fork arm
Fig. 1a: The RCX400 Telescope; Dec. Setting Circle (inset).
8
viewfinder
objective lens
2@
Fig. 1b: The Viewfinder close up.
2#
locking ring
2$
adjustment
screws
2%
viewfinder
eyepiece/focuser
viewfinder
bracket
2^
and dovetail
mount
A
Off/On
C
12vDC Out
tripod base with
2&
leg receptacles
leg
attachment
2*
lock
sliding leg
trigger
2(
release
tripod
legs
3)
Fig. 1c: The Tripod.
locking latch
and thruster bar
3!
mechanism
USB Ports
H
Ser
3@
J
ial por
T-handle
t
utoguider port
A
K
12vDC In
B
Fig. 1d: The Base Computer Control Panel.
USB P
D
AUX port
t
or
E
HBX por
F
t
Serial port
G
t
t accessor
Reticle port
L
Fig. 1e: The Optical Tube Assembly (OTA) Computer Control Panel.
HBX port
M
Smar
y por
N
9
Caution:
Using products other than
standard Meade accessories
may cause damage to the
telescope’s internal electronics and may void the Meade
warranty.
B Want to learn more
about the eyepieces
available for your
RCX400 telescope?
See OPTIONAL
ACCESSORIES
48, 49, and 50.
, pages
b Want to learn more
focusing your
about
telescope? See page
19.
h Want to learn how to
install the batteries?
See page 16.
i Want to lear
about the
Ascension and
Declination setting
circles
n more
Right
? See page 57.
RCX400: YOUR PERSONAL
WINDOW TO THE UNIVERSE
The Meade RCX400 models are extremely versatile, high-resolution telescopes. With
high-precision optics, pushbutton controls, precise GPS alignment, true-level and
North electronic sensors, automatic tracking of celestial objects, periodic error
correction f
the
Obser
Focus beyond the Solar System on ancient star clusters, remote galaxies, and stars
recently disco
are capable of meeting the requirements of the most demanding advanced observer.
or both axes, and a library of 145,000+ objects in the AutoStar II data base,
ve the feather structure of an eagle from 50 yards or split a difficult double star.
vered to have planets orbiting about them. Meade
RCX400 telescopes
B Eyepiece: Place the 2”, 6-element UltraWide 24mm eyepiece into the diagonal
mirror (
3, Fig. 1a) and tighten in place with the diagonal mirror’s thumbscrew (2,
Fig. 1a
). The eyepiece determines the magnification of the image collected in the
optical tube.
C 2" Diagonal Mirror and Eyepiece Thumbscrew: Provides a more comfortable
right angle viewing position. The eyepiece thumbscrew tightens the eyepiece (
) in place. Tighten to a firm feel only.
Fig. 1a
D Rear Cell P
The diagonal mirror slides into the visual back and is secured by the visual back
thumbscrew.
ort and 2” Visual Back:
The visual bac
k threads onto the rear cell.
1,
E Base Computer Control Panel (see j):
ON/OFF Switch: Turns both computer control panels and AutoStar II
A.
ON or OFF. The red power indicator LED next to the switch illuminates
when power is supplied to the panel and the AutoStar II handbox.
12vDC In: Provides a connection so that the telescope assembly may
B.
be powered from a standard 115v AC home outlet using the optional
RCX AC Wall Adapter with Cable or the optional 12v DC #607 Cigarette
Lighter Adapter. See
C.
12vDC Out: Use the 12vDC output to power telescope accessories.
This port may be turned on or off with the Aux Port Power option in the
Utilities menu. On is the default value.
USB 2.0 High Speed Port: Provides a connection for a USB 2.0
D.
device. This port is typically used to connect to a PC.
E.
AUX Port: Provides connection for current Meade accessories. See
OPTIONAL ACCESSORIES, pages 48 - 50.
Handbox (HBX) Port: Plug the AutoStar II coil cord into this port.
F.
tant Note:
Impor
the OTA Computer Control Panel include an HBX port, only one hand-
ybe be plugged in at a time;
x ma
bo
both ports at the same time.
G. Serial Port: Provides connection with a PC and for current and future
Meade accessories. Your PC can control your
serial commands. Go to the Meade website (www.meade.com) to
download the latest serial commands and device pinouts.
Important Note: Although both the Base Computer Control Panel and
TA Computer Control Panel include a serial port, only one may be
the O
used at a time; you cannot plug into both ports at the same time.
F Handles: Use to lift optical tube assemb
attached to the tripod. Attach the AutoStar II handbox holder to one of the handles (
5, Fig. 1a).
OPTIONAL ACCESSORIES, pages 48 - 50.
Although both the Base Computer Control P
you cannot plug handboxes into
RCX400 telescope using
ly or to rotate the telescope when
anel and
G Left Fork Arm: The left side of the heavy-duty mount that holds the optical tube
securely in place (see
1%).
H Battery Compartments: Insert four user-supplied C-cell batteries into each com-
tment (one compar
par
I Right Ascension (R.A.) Slo
Ascension, i.e., the horizontal axis, by turning this control with the R.A. Lock (see
tment on each f
w-Motion Control:
or
e fine adjustments in the Right
Mak
eight batter
m;
k ar
ies total).
10
Definitions
Throughout this manual,
you will notice the terms
Alt/Az," "Right
"
Ascension
Declination." Alt/Az or
"
more properly, altitudeazimuth (or altazimuth), is
frequently used to refer to
altitude or Declination (the
up-and-down vertical movement of the telescope) and
azimuth or Right Ascension
(the side-to-side horizontal
movement of the telescope). Right Ascension is
abbreviated as "R.A." and
Declination as "
Caution:
When loosening the Dec.
lock, be sure to support the
optical tube (19,
The weight of the tube
could cause the tube to
swing suddenly.
," and
Dec."
Fig.
1a
).
1#) in the unlocked position. Set the R.A. Lock to a "partially locked" position to create
ortable drag for the R.A. Slow Motion Control.
a comf
Caution: Do not oper
in the fully locked position, as such operation may result in damage to the
internal gear system and also cause you to lose alignment.
ate the R.A. Slow Motion Control with the R.A. Lock
j Optical Tube Assembly (OTA) Computer Control Panel (also see e):
H. USB Port: Provides 3 connections for USB 2.0 devices. This port is
typically used to connect to CCD cameras, such as Meade’s LPI or
Deep Sky Imager
PC can control your
the Meade website (www.meade.com) to download the latest serial
commands and de
J. Serial Port: Provides connection with a PC and for current and future
Meade accessories. Your PC can control your
serial commands. Go to the Meade website (www.meade.com) to
wnload the latest serial commands and device pinouts.
do
Important Note: Although both the Base Computer Control Panel and
the OTA Computer Control Panel include a serial port, only one may be
used at a time; you cannot plug into both ports at the same time.
K. Autoguider Port: Plug the optional autoguider into this port. See the
instruction sheet that came with your autoguider for more information.
Also see OPTIONAL ACCESSORIES, pages 48 - 50.
L. Reticle Port: Plug the optional reticle eyepiece into this port. Control
the reticle through the AutoStar II menus. See
page 36. Also see OPTIONAL ACCESSORIES, pages 48 - 50.
Note: See the instruction sheets that are included with the reticle and
the autoguider for more details.
M. Handbox (HBX) Port: Plug the AutoStar II coil cord into this port.
Important Note: Although both the Base Computer Control Panel and
the OTA Computer Control Panel include an HBX port, only one handbox maybe be plugged in at a time; you cannot plug handboxes into
both ports at the same time.
N. Smart Accessory Port: Provides connection for future Meade acces-
sories.
. See
OPTIONAL ACCESSORIES, pages 48 - 50.Y
RCX400 telescope using serial commands. Go to
vice pinouts.
RCX400 telescope using
HOT BUTTON MENUS
our
1) GPS Receiver: Receives information transmitted from Global Positioning System
satellites. See page 25 for more information.
1! Declination (Dec.) Setting Circle (on left fork arm): See APPENDIX A, page 57,
for detailed information.
1@ Mounting Base: Attach to the tripod base (see 2&). See page 16 for mounting
instructions.
1# Right Ascension (R.A.) Lock: Controls the manual horizontal rotation of the
telescope.Turning the R.A. lock counterclockwise unlocks the telescope, enabling
it to be freely rotated b
kwise loc
cloc
ally, and engages the horizontal motor drive for AutoStar II operation.
utoStar II Handbo
1$ A
of the telescope. See pages 13 - 15 for detailed information. You may have
noticed that there is no manual focus knob; all focus is achieved by
utoStar handbo
A
handbox in a convenient location.
ks the telescope
1% Right Fork Arm: The r
tube securely in place (see
1^ Dec
lination (Dec.) Slo
Declination(altitude) by turning this control with the Dec. Lock (see
ed position. In order for this control to operate properly, power must be off.
k
the loc
y hand about the horizontal axis. Turning the R.A. lock
, prevents the telescope from being rotated manu-
le Holder:
Tiltab
x and
Attach the holder to one of the handles (see
x.
ight side of the hea
g).
w-Motion Contr
Controls all the electronic functions
vy-duty mount that holds the optical
ol:
e fine adjustments in
Mak
using the
Holds y
f).
1& below) in
our
1& Dec. Lock: Controls the manual vertical movement of the telescope. Turning the
k countercloc
loc
Dec.
by hand about the vertical axis. Turning the Dec. lock clockwise (to a firm feel
kwise unloc
ks the telescope enabling it to be freely rotated
11
2! Want to learn more
about attaching and
aligning the
viewfinder
18.
? See page
only) pre
cal motor drive for AutoStar II operation.
1* Dust Co
Note: The dust cover should be replaced after each observing session and the
power turned off to the telescope.
vents the telescope from being moved manually, but engages the verti-
ver:
Gently pr
y the dust cover from the front lens of the telescope.
1( Optical Tube: The main optical component that gathers the light from distant
objects and brings this light to a focus for examination through the eyepiece.The
tube contains the primary mirror which floats on a layer of adhesive that results
in zero-stress to the glass and no distortion to the optics.
2) Fan: AutoStar controls the fan operation. The amount of time required to stabi-
e the temperature will be dependent upon ambient conditions including the
liz
observation site and preexisting condition of the telescope. The fan should be
activated at the beginning of the observation session to accelerate the temperature stabilization. As soon as the optics have reached an equilibrium with the
environment the fan should be turned off. Fan operation time should range
between 5 and 25 minutes. While it is permissible to run the fan continuously it is
not recommended because the very slight vibration of the fan may cause noticeable movement of the objects observed in the sensitive optics.
The Viewfinder
2! 8 x 50mm Viewfinder: A low-power, wide-field sighting scope with crosshairs
that enables easy centering of objects in the telescope eyepiece.
2@ Viewfinder Objective Lens: Gathers the light for the viewfinder.
2# Viewfinder Locking Ring: Locks the objective lens into place. Unlock to adjust
the focus of the objective lens. See page 18 for details.
2$ Viewfinder Adjustment Screws: Use these six screws to adjust the alignment
of the viewfinder.
2% Viewfinder Eyepiece/Focuser: The eyepiece magnifies the image collected by
the viewfinder’s objective lens. Rotate the eyepiece to focus.
2^ Viewfinder Bracket and Mounting: Holds the viewfinder in place.
The Tripod
2& Tripod Base with leg receptacles: Attach the mounting base (see 1@) to the tri-
pod base. See page 16 for mounting instructions. Slide the tripod legs into the leg
receptacles.
2* Leg Attac
hment Lock (3):
Secures the tr
ipod legs into the leg receptacles.
2( Sliding Leg Trigger Release and pin: Press and hold down this lever to easily
change the length of the tripod legs. Let go of the trigger when the tripod leg is
at the desired length. The Trigger has a pin that runs through the mounting base;
this pin attaches to the thr
uster latch (see
3! belo
w).
3) Variable Height Tripod Legs: Supports the optical tube assembly.
See page
3! Thruster Latc
16 for mounting instructions. Also see
h:
Attach to tr
igger release pin to secure tr
Fig. 8).
ipod in place
.
3@ T-Handle: Thread into the mounting base and tighten to a firm feel to keep the
tripod stable.
12
AUTOSTAR II FEATURES
K
1
Want to learn more about
downloading the latest
updates of Autostar II
software from the
Meade website
www.meade.com/support/auto.html for complete instructions. Also
see page 43.
? Go to
2
4
3
8
5
6
7
Fig. 2: The Autostar II Handbox.
Tour the Cosmos with Just the Push of a Button
Control of the RCX400 telescope models is through the operation of the standard
Autostar II system. Nearly all functions of the telescope are accomplished with just a
few pushes of Autostar II’s buttons.
Because the Autostar II system uses flash (rewritable) memory, your system will be
able to grow when new features and enhancements become available. Download the
latest satellite data, star and object catalogs, tours, serial commands list, and software
revisions, directly from the Meade website (
RCX400 Interface Cable. See OPTIONAL ACCESSORIES, pages 48 - 50.)
al
Some of the major features of the Autostar II system are:
JAutomatically move the telescope to any of the more than 180,000 objects stored
in the object library, including:
Library# of Objects
New General Catalog (NGC):7,840
Index Catalog (IC):5,386
Messier Catalog (M):110
ell Catalog:
Caldw
Named Objects:
Herschel Catalog:
Abell Catalog of Galaxy Clusters:
Arp Catalog of Irregular Galaxies:645
Uppsala Galaxy Catalog:
phological Catalog of Galaxies:
Mor
al Catalog of
Gener
SAO:17,191
Hipparcos Star Catalog:
....plus the Lunar 100, the Washington Star Catalog, the Gliese Catalog, and more!
our telescope’
ocus y
JF
ake a guided tour of the best celestial objects to view on any given night of the year.
JT
JControl your RCX400 with your PC using an RS232 or USB interface.
JAlign your telescope automatically using GPS (Global Positioning System).
JAccess a glossary of astronomical terms.
JMount the telescope in the
vertical—horizontal mode) for fully automatic tracking of celestial objects.
JCollimate your telescope using only AutoStar II’s Arrow keys.
Variable Stars:28,484
s eyepiece.
www.meade.com). (Requires the option-
109
227
400
2,712
12,940
12,939
17,325
“Alt/Az”
mode (i.e, altitude—azimuth, or
9
J
13
e Want to learn more
about using the GO TO
function? See page 24.
ant to learn how to
W
m a
or
perf
search? See page 24.
SPEED
1
about c
speeds? See page 21.
spiral
Want to learn more
hanging sle
utostar II system provides control of virtually every telescope function. The
The A
Autostar II handbox has soft-touch keys designed to have a positive feel. The LCD
(Liquid Crystal Display) is backlit with red LEDs (Light Emitting Diodes) for easy viewing in the dark. The backlit display, key arrangement, and sequential menu structure
e Autostar II extremely user friendly.
mak
B 2-Line LCD Display: This screen displays Autostar II's menus and information
about the telescope.
•
Top line: Lists the primary menu.
• Bottom line: Displays other menus that may be chosen, menu options,
telescope status
formed.
, or information about a function that is being per-
c ENTER Key: Press to go to the next menu level or to choose an option in a menu.
The ENTER key is similar to the RETURN or ENTER key on a computer. See
MOVING THROUGH AUTOSTAR II'S MENUS, page 22 and BASIC AUTOSTAR II
OPERATION, pages 26 - 27
d MODE Key: Press to return to the previous menu or data level. The top menu
level is “Select Item." The MODE key is similar to the ESCAPE key on a computer.
Note: Pressing MODE repeatedly while in the “Select Item” level moves
Autostar II to the topmost screen: “Select Item: Object.”
Note: If MODE is pressed and held for two seconds or more, information
about the telescope's status displays.When the status displays, press the
Scroll keys (
• Right Ascension and Declination (astronomical) coordinates
• Altitude (vertical) and Azimuth (horizontal) coordinates
• Local Time and Local Sidereal Time (LST)
• Timer and Alarm Status
• Date
• Site coordinates
• Battery status
Press MODE again to return to the previous menu.
7, Fig. 2) to display the following information:
e GO TO Key: Press to slew (move) the telescope to the coordinates of the cur-
rently selected object. While the telescope is slewing, the operation may be aborted at any time by pressing any key except GO TO. Pressing GO TO again
resumes the slew to the object. Also, press during the alignment or GO TO procedures to activate a "spiral search."
f Arrow Keys: The Arrow keys have several functions. Press an Arrow key to slew
the telescope in a specific direction (up, down, left, and right), at any one of nine
different speeds. See
to move the telescope vertically up and down. The Left Arrow key rotates the tele-
ontally counterclockwise, while the Right Arrow key rotates it clockwise
scope hor
(unless reversed for Southern Hemisphere use).
Also
The Down Arrow key begins with the letter "A;" the Up Arrow key begins with digit
"9."
Additionally
Right or Left Arrow key (
in the display.
g Number K
w
ic function, which is printed on each key (these are commonly known as "hot buttons"—see page 36):
iz
, use the Arro
, use the Arrow keys to move the cursor across the display: Use the
eys:
1 SPEED: Changes the slew speeds. To operate, press Speed and then a
Number key (1 is the slowest speed, 9 is highest speed).
2 CALD (Caldwell): Press to display the Caldwell catalog on the Autostar II
handbox.
3 M (Messier): Press to display the Messier catalog library.
SLEW SPEEDS, page 21. Use the Up and Down Arrow keys
eys to scroll through numbers 0 through 9 and the alphabet.
w k
5, Fig. 2) to move the cursor from one number to the next
Press to
input digits 0 to 9. Each Number key also has a specif-
14
FOCUS
4
Want to learn
more about the
? See page 19.
menu
RET
7
Want to learn
more about the
menu? See page 36.
Focus
Reticle
4 FOCUS: Toggles between two functions. The first press allows you to
change the focus and focus speed. The next press allows you to create
presets that tell the telescope where to f
ocus.
5 SS: Press to display the Solar System library.
6 STAR: Press to display the Star library.
7 RET (Reticle):
Press to display the Reticle Control menu.
8 IC: Press to display the Index Catalog library.
9 NGC (New General Catalog): Press to display the NGC catalog library.
0 LIGHT: Press to turn on and off the red utility light on the top of the hand-
box.
h Scroll Keys: Press to access options within a selected menu. The menu is dis-
played on the first line of the screen. Options in the menu are displayed, one at a
time, on the second line. Press the Scroll keys to move through the options. Press
and hold a Scroll key to move quickly through the options.
The Scroll keys also control the speed of text scrolling on the Autostar II display.
When text is scrolling, press and hold the Up Scroll key for a faster display speed
and the Down Scroll key for a slower display speed.
Tip:
When an astronomical
appears in [brack-
term
], press ENTER for a
ets
definition or more detailed
information. Press MODE
to return to the scrolling
Autostar II Help display.
celestial object's
If a
name appears in brackets
(and your telescope is
aligned), press ENTER
and then GO TO to slew
the telescope to the object.
i ? K
ey:Press to access the "Help" file. "Help" provides on-screen information on
how to accomplish whatever task is currently active.
Press the ? key and then follow the prompts on the display to access details of
Autostar II functions in the Help feature. The Help system is essentially an onscreen instruction manual.
If you have a question about an Autostar II operation,
ALIGNMENT,
etc., press the ? key and follow the directions that scroll on the sec-
e.g., INITIALIZATION,
ond line. When satisfied with the Help provided, press MODE to return to the original screen and continue with the chosen procedure.
j Coil Cord Port: Plug one end of the Autostar II coil cord (10, Fig. 2) into this port
located at the bottom of the Autostar II handbox.
1) Coil Cord: Plug one end of the Autostar II coil cord into the HBX port (F, Fig. 1d)
of the computer control panel of the telescope and the other end into the Autostar
II coil cord port. See
j above.
1! Utility Light: Use this built-in red light to illuminate star charts and accessories
without disturbing your eye's adaptation to darkness. Press "0" to turn the light on
and off.
RCX400 TIPS
Join an Astr
One of the best ways to increase your knowledge of astronomy is to join an astronomy
club. Check your local newspaper, school, library, or telescope dealer/store to find out if
s a club in y
there’
At club meetings
to share your discoveries. Clubs are an excellent way to learn more about observing the
sky, to find out where the best observing sites are, and to compare notes about tele-
, eyepieces, filters, tripods, and so forth.
scopes
Often, club members are excellent astrophotographers. Not only will you be able to see
examples of their art, but you may even be able to pick up some “tricks of the trade” to
try out with your
phy with the
y g
Man
observe with many different telescopes and other pieces of astronomical equipment.
Magazines such as
Star Parties around the United States and Canada.
RCX400.
roups also hold regular
onomy Club, Attend a Star Party
our area.
ou will meet other astronom
, y
RCX400 telescope. See page 45 for more information about photogra-
ly scheduled Star P
Sky & Telescope and Astronomy print schedules for many popular
y enthusiasts with whom you will be able
arties at which you can check out and
15
GETTING STARTED
Fig. 7: Attach leg (1) to leg
receptacle (2).
Fig. 8: Rotate the leg until the trigger
release pin (4) is next to the thruster
bar (3).
f
Fig. 9: Slide thruster hook (4) into
the slot of the trigger release pin (3).
Fig. 10: Tighten the leg adjustment
loc
Fig. 11: Press down the trigger lever
(5) so that you can adjust the height
of the tripod.
16
k (6).
d
f
g
c
B
e
d
e
Parts Listing
Getting the telescope ready for first observations requires only a few minutes. When
first opening the pac
JRCX400 Telescope with fork mount system and GPS Receiver
JAutoStar II handbox and interface coil cord; handbox holder
J8 x 50mm viewfinder assembly
J2" diagonal mirror and
JSeries 5000 UltraWide 24mm eyepiece
ariable height tripod
JV
JUSB cable and software CD ROM
king box, note carefully the following parts:
2” visual back barrel
How to Assemble the Tripod
Remove the parts of the tripod from the shipping carton. Assembly of the tripod will
take just a few minutes.
To assemble the tripod:
1.Slide a tripod leg into a leg receptacle (Fig. 7). Rotate the leg until the trigger
release pin is next to the thruster bar latch (
2.Slide the thruster bar latch hook into the slot in the trigger release pin (
3.Rotate the leg attachment lock to tighten the leg in place (
4.To unlock the leg, press and hold down the trigger release lever (
holding the lever down, slide the leg extension in or out to the desired length. Let
go of the lever to lock the leg extension into place. Unhook the trigger release pin
to lock the leg in place.
5.Repeat steps 1 through 4 for the other two tripod legs.
Fig. 8).
Fig. 9).
Fig. 10).
Fig. 11). While
How to Assemble Your Telescope
The telescope’s fork mounting base attaches directly to the tripod. The telescope in
this way is mounted in an “altazimuth” (“altitude-azimuth,” or “vertical-horizontal”) format. It is recommended that two people attach the mount to the tripod.
Caution for 12” and 14” model users: Due to the weight and size of
these products, please use extreme caution whenever assembling,
disassembling, lifting, transporting or storing these products. Two or more
persons should always be used whenever performing any of these tasks.
Disregard for the above warning could result in serious injury or death.
Note: The field tr
equatorial wedge (see your wedge’s instruction sheet for more
mation) f
or
inf
ipod base comes with a tangent ar
The tr
To attach the mount:
1.Take note of the T-handle under the tripod base. The T-handle is spring-mounted
into position. Note also that there is a hole on the bottom side of the mount base.
2.Lift the mount and position the mount base over the tripod base. Line up the hole
on the mount base o
mount do
3.Rotate the T-handle until the rod is tightened to a firm feel (
To install the batteries:
Assembly of the RCX400 telescope requires eight C-cell (user-supplied) batteries or
the optional RCX A
into the 12vDC In por
1.Turn the Dec. lock (
(
19, Fig. 1a). Move the optical tube to the position depicted in Fig. 1a and turn
the Dec. lock clockwise to a firm feel to relock the position of the optical tube.
2.Remove the battery compartment covers (
batter
supplied C-cell batter
gram on the battery slots inside the battery holder. Return the battery holders to
their respectiv
wn onto the rod and the rod will “pop up” into the hole (
y holders, being mindful of the connector wires (
ipod also can be used in conjunction with the optional
or long exposure astrophotography.
m attached f
ver the T-handle rod. When they are lined up, place the
Wall Adapter to a standard 115v home outlet . Plug the adapter
C
t of the computer control panel (
17, Fig. 1a) counterclockwise to unlock the the optical tube
ies into each batter
e compar
tments and replace the co
y holder
or use with the superw
Fig. 13).
Fig. 1d
B,
7, Fig. 1a) and carefully remove the
, or
ers.
v
).
Fig.15).
iented as sho
edge
Fig.12).
Insert four user-
wn on the dia
.
-
Caution: Use care to install batter
compartment. Follow battery manufacturer's precautions. Do not install
ies backwards or mix new and used batteries. Do not mix battery
batter
types. If these precautions are not followed, batteries may explode, catch
, or leak. Improperly installed batteries void your Meade warranty.
fire
Always remove the batteries if they are not to be used for a long period of
time.
To attach AutoStar II and connect the handbox holder
ies as indicated by the battery
h
i
Fig. 12: Line up the T-handle rod (8)
with the hole on the base (7).
j
Fig. 13: Tighten the T-handle (9) to a
“firm feel.”
1!
1)
1$
1@
16:
Fig.
Locations of the On/Off s
HBX por
ed on the base of the telescope
1.Plug in the AutoStar II handbox: Check that the power switch on the computer
2.Attach the handbox holder: Remove the handbox holder from the plastic bag. If
To attach the diagonal mirror and the eyepiece
t on the Computer Control Panel locat-
control panel (
II handbox into the HBX port of the base control panel (
port of the OTA control panel (
Note: The AutoStar II handbox does not require batteries; the batteries in
the telescope supply the power.
Note: You can only plug one handbox into the telescope at a time; you
cannot plug in two handboxes into the two control panels at the same time.
necessary, loosen the lock knob (
about one of the fork arm handles (
feel. Slide the AutoStar II handbox into the holder (
snap the handbox into the holder: Slide one side of the handbox into the holder
and then firmly press the other side of the handbox into the holder until it snaps
in place. Adjust the tilt of of the holder by loosening the lock knob and then moving the holder clamp to the desired angle. Retighten the lock knob.
12, Fig. 16) is in the OFF position. Plug the coil cord of the AutoStar
1#
witch and the
.
M, Fig. 1e).
14, Fig. 17a) and place the clamp (15, Fig. 17a)
A
Fig. 17a: Handbox holder: (14) Lock
knob; (15) Clamp; (16) Holder.
Fig. 17b: Handbox holder attached to
fork arm handle.
15, Fig. 1a). Tighten the lock knob to a firm
1%
1^
16, Fig. 17a).You may also
B
13, Fig. 16) or the HBX
Fig. 14: Loosen the R.A. (11) and
Dec.
tube from its shipping position.
Fig. 15: Battery installation.
ks to Move the optical
(10) loc
1&
1&
1(
1*
18:
Fig.
Rear cell
(17).
Visual bac
Attach
1.
the rear cell and rotate the ring, tightening to a firm feel (see
Slide the diagonal into the visual bac
thumbscrew.
19:
Fig.
visual back (18) onto the rear
cell (17). Slide diagonal into the
visual bac
thumbscrew (19).
k and Diagonal mirror
Thread the r
k and secure with
ing of the
Thread the ring of the visual back over
:
k and secure it in place using the visual bac
2)
2!
epiece (20)
y
Slide e
Fig.20:
into the diagonal mirror and
tighten thumbscrew (21).
Figs. 18 and 19) .
k
17
2#
2$
Fig. 21: Viewfinder bracket assembly:
Slide the track (23) into the mounting
slot (22). Tighten the thumbscrews
(24) to secure.
2%
2&
Fig.22: 8x50 Viewfinder tube:
Objective lens (25), eyepiece/focuser
(26) and locking ring (27).
2*
2@
2^
2.Insert eyepiece: Remove the UltraWide 24mm eyepiece from its container and
slide it in the diagonal mirror. Tighten the thumbscrew (
diagonal mirror to a firm feel only.
3.Remove dust cover: Remove the dust cover (
assembly by gently prying it off.
18, Fig. 1a) from the optical tube
Fig. 20) located on the
Mounting and Focusing the Viewfinder for the First Time
The first time you mount and focus the viewfinder, follow the these steps:
1.Slide the track on the bottom of the viewfinder bracket into the slot in the viewfinder mounting assembly. See
assembly, tighten the two thumbscrews to a firm feel only.
Slide the viewfinder tube (see
2.
en the adjustment screws (see
align the viewfinder (see the next section below).
2.Look through the viewfinder. Rotate the eyepiece/focuser until you sharply focus
the crosshairs.
3.Loosen (rotate clockwise) the objective lens locking ring.
4.Rotate the objective lens until you sharply focus on an object located at infinity.
5.Tighten the locking ring.
6.You may now rotate the eyepiece to focus on objects.
Fig. 21. To secure the viewfinder to the mounting
Fig.22) into the vie
Fig. 23). You will use the adjustment screws to
wfinder bracket. Loosely tight-
Aligning the Viewfinder
To align the viewfinder, perform steps 1 through 4 during the daytime; perform step 5
at night.
1.If you have not already done so, insert the UltraWide 24mm eyepiece into the
diagonal mirror.
2.Unlock the R.A. (
moves freely on both axes.
3.Point the telescope at some well-defined and stationary land object at least 200
yards distant, such as the top of a telephone pole or street sign. Center the object
in the telescope eyepiece. Re-tighten the R.A. and Dec. locks.
4.Look through the viewfinder eyepiece and loosen or tighten, as appropriate, one
or more of the viewfinder adjustment screws (see
crosshairs are precisely centered on the object you previously centered in the telescope eyepiece.
5.Check this alignment on a celestial object, such as the Moon or a bright star, and
y necessar
e an
mak
Note: Seeing conditions v
urbulence in the air, even on an apparently clear night, can distort
T
images. If an image appears fuzzy and ill-defined, back off to a lower
er e
w
po
13, Fig. 1a) and Dec. (17, Fig. 1a) locks so that the telescope
Fig. 23) until the viewfinder
, using the method outlined in steps 2 through 4.
y widely from night-to-night and site-to-site
ar
ell-resolved image (see
24a and 24b
Fig.
epiece f
y
y refinements
or a more w
.
).
Fig. 23: Viewfinder adjustment screws
(28).
Fig. 24a & 24b: Jupiter; examples of
the right amount of magnification and
too much magnification.
18
RCX400 TIPS
oo Much Power?
T
Can you ever have too much power? If the type of power you’re referring to is
epiece magnification, y
y
e
ning obser
the telescope’
Keep in mind that a smaller, but bright and well-resolved image is far superior to
one that is larger, but dim and poorly resolved (see
abo
tions.
utostar II can calculate the best e
A
Calc” feature in the Utilities menu.
Most obser
ange of reasonab
r
OPTIONAL ACCESSORIES, pages 48 - 50.
ver is to “overpower” a telescope by using high magnifications which
s aper
e 400X should be employed only under the steadiest atmospheric condi-
v
ers should ha
v
le magnifications possible with the
, you can! The most common mistake of the begin-
es
ture and atmospheric conditions cannot reasonably support.
Figs. 24a and 24b). Powers
epiece for you to use. Try out the “Eyepiece
y
e three or f
v
our additional eyepieces to achieve the full
RCX400 telescopes
.
See
Important Note:
Objects appear upside-down
and reversed left-for-right
when observed in the
viewfinder. Objects viewed
through the telescope eyepiece when inserted into the
diagonal prism assembly
appear right-side-up, but
reversed left-for-right.
This image inversion is of no
consequence when observing astronomical objects and,
in fact, all astronomical telescopes yield inverted
images.
During terrestrial observing,
where a fully-correctly-oriented image (right-side-up and
correct left-for-right) is desirable, an optional #928 45°
Erecting Prism and optional
1.25” eyepiece holder are
available. See
ACCESSORIES, pages 48 -
50.
OPTIONAL
OBSERVING
Choosing an Eyepiece
A telescope’s eyepiece magnifies the image formed by the telescope’s main optics.
Each eyepiece has a focal length, expressed in millimeters, or “mm.” The smaller the
focal length, the higher the magnification. For example: An eyepiece with a focal
length of 9mm has a higher magnification than an eyepiece with a focal length of
26mm.
Your telescope comes supplied with an UltraWide 24mm eyepiece which gives a
wide, comfortable field of view with high image resolution.
Low power eyepieces offer a wide field of view, bright, high-contrast images, and eye
relief during long observing sessions. To find an object with a telescope, always start
with a lower power eyepiece such as the UltraWide 24mm. When the object is located and centered in the eyepiece, you may wish to switch to a higher power eyepiece
to enlarge the image as much as practical for prevailing seeing conditions. For information about optional eyepieces for your telescope, see
pages 48 - 50.
The power, or magnification of a telescope is determined by the focal length of the telescope and the focal length of the eyepiece being used (an eyepiece's focal length is
printed on the side of the eyepiece). To calculate eyepiece power, divide the telescope's focal length by the eyepiece's focal length.
supplied with
SPECIFICATIONS, pages 54 - 56).
RCX400 models. The focal length of the 12" f/8 RCX400 is 2438mm (see
Eyepiece Power = Telescope focal length ÷ Eyepiece focal length
Eyepiece Power = 2438mm ÷ 24mm
Eyepiece Power = 102
The eyepiece power, or magnification is therefore 102X (approximately).
Note: For a list of magnification ratings of the eyepieces available for the
RCX400 telescopes, see OPTIONAL ACCESSORIES, pages 48 - 50.
OPTIONAL ACCESSORIES,
For example: A 24mm eyepiece is
FOCUS
KEY
Fig. 25: Focus is all-digital, using the
Focus key (the #4 Number key) of
the AutoStar II handbox.
Focusing the Telescope
All focusing of the RCX400 is performed digitally, using AutoStar II’s Focus key
(number key 4). The Focus key functions as a toggle key:
J Press the Focus key the first time to focus the telescope eyepiece and to control
the speed at which you focus.
J Press the Focus key again to set and adjust up to nine focus presets.
To change the focus speed:
1.Press the Focus key once. “Focuser: Fast (or the current speed)” displays for
two seconds. Use one of the Scroll keys to scroll through the list of 4 available
focus speeds: Fast, Medium, Slow, Fine. Scroll through the list until the speed
. Choose a focus speed with which you feel comfortable.
ou desire displa
y
To focus the telescope eyepiece:
1.Press the Focus key once. “Focuser: Fast (or the current speed)” displays. After
two seconds, “Focuser: Position = XX” displays. “XX” stands for a number value
in decimal millimeters
2.Point the telescope at a distant object. Look in the eyepiece and use the Arrow
keys until the image in the eyepiece is in sharp focus.
Presets:
ou “Park” your telescope, you do not have to refocus the telescope each time you
If y
use it. Nine preset focus positions are available, and they operate much like presets
on a car radio—everyone can have their own favorite station, or in this case, their own
personalized focus. You can set one preset to take into account your own eyesight,
or your observing partner (who may wear glasses), one for your camera’s focus,
one f
and so forth.
Three preset menus are available. Use the Define Preset menu to assign a preset,
use the GoTo Preset menu to select a preset you have previously assigned, and use
ys
.
19
Note:
Viewing conditions vary widely from night-to-night and siteto-site. Turbulence in the air,
even on an apparently clear
night, can distor
Low-power e
as the UltraWide 24mm supplied with your telescope, are
better suited to resolving
images in poor viewing conditions.
t images.
yepieces, such
Sync On Preset men
focus presets after you turn off and turn on your scope again ).
To define a preset:
Point the telescope at a distant object, press FOCUS and use the Up and Down
1.
Arrow keys to focus the telescope until the object is sharply focused as previously
xplained.
e
2.Press the Focus key again (FOCUS toggles between the Focus menu and the
Preset menu). “Focuser Preset: Go To” displays. Use a Scroll key and scroll down
the list of options until “Focuser Preset: Define Preset” displays. Press ENTER.
3.A list of presets displays. If no preset is currently assigned, “1- Unnamed” displays
ollowed by 2- Unnamed, up to 9 - Unnamed).
(f
4.Use the up and down Scroll keys to scroll through the alphabet and the right and
left Arrow keys to move to cursor right or left across the display.
5.When you have finished typing in a name and focusing the telescope, press
ENTER. That number preset is now defined. You can enter 9 names. For example, you may enter “Joe,” “Jill,” “Deep Sky Imager” and so forth.
6.To select one of these presets, you will use the “Focuser Preset: Go To” menu.
To select a previously defined focus preset
1.Press the Focus key twice. “Focuser Preset: Go To Preset” displays. Press
ENTER to select this menu.
2.Use a Scroll key and scroll down the list of previously defined presets. When the
desired preset displays (for example, “Deep Sky Imager”), press ENTER.
Important Note: If you do not park your telescope, you will need to select
one of the presets and refocus your telescope using the Sync On menu.
TO SYNC ON A FOCUS PRESET below.
See
To sync on a focus preset
If you park your telescope, AutoStar II remembers all the focus positions you
defined as presets and you will not need this menu.
If you do not park your telescope, you will need to select just one of the presets and
refocus your telescope using the Sync On menu. Then AutoStar II will then reset all
the other presets back to the focus preset positions you previously defined.
1.Press the Focus key twice. “Focuser Preset: Go To Preset” displays. Use a Scroll
key and scroll until “Focuser Preset: Sync On Preset” displays and press ENTER
to select this menu.
2.Use a scroll key to choose one of the previously entered presets from this list (the
most likely preset you will choose will be one that accounts for your own
eyesight).
Use the Up or Do
3.
4.Press ENTER. AutoStar II now “remembers” the relative focus positions of the
yepiece.You can now choose any preset and it will be correctly focused.
e
To exit the focus operation at any time:
1.Press MODE.
u if you do not park your telescope (this menu will reset all your
wn Arrow keys to focus the eyepiece.
Observing by Moving the Telescope Manually
If you wish to observe a distant land object, such as a mountain top or a bird, you can
observe by merely pointing the telescope and looking through the eyepiece.
1.Loosen the telescope’s R.A. lock (
2.Move your telescope to observe distant street signs, mountains, trees, and other
structures. Use your viewfinder to help site-in on an object.
3.Center the object in the viewfinder’s crosshairs and then in the telescope eye
When the object is
.
piece
R.A. and Dec. locks.
4.To move telescope in the R.A. and Dec. axes again, remember to loosen the R.A.
lock and tighten the Dec. lock. Then rotate the manual slow motion control knobs
(
10, Fig. 1a) and (16, Fig. 1a) .
5.Practice digitally focusing on objects.
See FOCUSING THE TELESCOPE, page 19.
6.Once you get a feel for how your telescope moves and focuses, try to view some-
centered in your eyepiece, remember to re-tighten the
13, Fig. 1a) and Dec. lock (17, Fig. 1a).
20
NEVER point
the telescope
directly at or
any time! Observing the
Sun, even for the smallest
fraction of a second, will
result in instant and irreversible eye damage, as
well as physical damage
to the telescope itself.
Warning:
Do not look through the telescope's eyepiece or viewfinder while it is rapidly moving.
Children should always have
adult supervision while
observing.
Tip:
The slowest speed, 1x,
ma
Guiding Rate menu. This
men
the speed by entering a
percentage of the speed
(either more or less than
100%). This function may
be useful in guiding the tel
escope during CCD and
long-e
See
34, f
near the Sun at
y be changed using the
ws you to change
u allo
aph
mation.
or
r
xposure photog
GUIDING RATE, page
or more inf
You can also observe stars and objects in the night sky using this method, but note
that objects begin to slowly drift across the eyepiece field. This motion is caused by
the rotation of the Earth. As you become familiar with the Autostar II handbox operation, you can counteract the drift using the automatic tracking feature in the Autostar
II Setup menu (see
Autostar II's GO TO capabilities (see
TO TRACK AN OBJECT AUTOMATICALLY, page 22), or by using
GO TO SATURN, page 24).
Terrestrial Observing
The RCX400 models are excellent high-resolution terrestrial (land) telescopes.
Viewing terrestrial objects requires looking along the Earth's surface through heat
aves.These heat waves often cause degradation of image quality. Lower power eye-
w
pieces, like the UltraWide 24mm, magnify these heat waves less than higher power
eyepieces.Therefore, lower power eyepieces provide a steadier, higher quality image.
If the image is fuzzy or ill-defined, reduce to a lo
wer power eyepiece, where the heat
waves do not have such an effect on image quality. Observing in early morning hours,
before the ground has built up internal heat, produces better viewing conditions than
during late afternoon hours.
Observing Using Autostar II's Arrow Keys
You may observe land and astronomical objects using Autostar II's Arrow keys to
move the telescope.
1.Tighten the R.A. and Dec. locks (
2.Verify that Autostar II is properly connected to your telescope. See
AUTOSTAR
II,
page 17.
13 and 17, Fig. 1a).
TO CONNECT
3.Flip the telescope power switch to the ON position.
The Autostar II screen is activated and a copyright message displays briefly, followed
by a short beep. Then Autostar II takes a few moments to start up the system.
4.A message displays that warns not to look at the Sun. At the end of this mes-
sage, press the key prompted by Autostar II to signify that the message has been
read and understood.
5."Automatic Alignment" displays.
6.The Arrow keys are now activated. Press the Arrow keys (
5, Fig. 2) to slew
(move) the telescope up, down, right, or left.
7.Press the Speed key (Number key "1") and then a Number key (
6, Fig. 2) to
change the telescope’s slew speed. ("1" is the slowest speed, "9" is highest
speed.)
8.Use the viewfinder (
21, Fig. 1a) to locate an object and practice using the
Autostar II’s Arrow keys to center the object in the telescope’s field of view.
9.Bring the object into focus.
Slew Speeds
Autostar II has nine slew speeds that move the optical tube at rates that are directly proportional to the sidereal rate and have been calculated to accomplish specific functions.
Press the Speed key (Number key "1") and then press a Number key to change the slew
speed, which is shown for about two seconds on Autostar II’s display.
ailable speeds are:
The nine a
-
.
y
v
Number Key 1 =1x =Guide Rate, programmable (see
2x =2 x sidereal (0.5 arc-min/sec or 0.008°/sec)
=
y 2
Number K
Number K
e
x sidereal (2 arc-min/sec or 0.033
8x =
=
y 3
e
8
Tip at left)
/sec)
°
Number Key 4 =16x =16 x sidereal (4 arc-min/sec or 0.067°/sec)
Number K
Number K
e
/sec
arc-min/sec or 0.5
128x =
=
y 6
e
30
°
64x =64 x sidereal (16 arc-min/sec or 0.27°/sec)
=
y 5
Number Key 7 =1.5° =90 arc-min/sec or 1.5°/sec
3° = 180 arc-min/sec or 3°/sec
=
y 8
Number K
Number K
e
arc-min/sec or 8
Max =
=
y 9
e
480
°/sec)
Speeds 1, 2, or 3: Best used for fine centering of an object in the field of view of a
er eyepiece, such as a 12mm or a 9mm eyepiece.
higher po
w
21
Definition:
Initialization
dure that ensures that
Autostar II operates correctly. When you first use
Autostar II, it doesn't yet
know where the observation location site is or the
time or date of the observation session.
During the
alignment procedure, the
system calculates these
parameters automatically.
Autostar II uses this information to precisely calculate the location of celestial
objects (such as stars and
planets) and to move your
telescope correctly for various operations.
is a proce-
automatic
Speeds 4, 5, or 6: Enable centering of an object in the field of a low-to-moderate
wer eyepiece, such as the standard UltraWide 24mm.
po
Speeds 7 or 8: Best used for rough centering of an object in the viewfinder.
Speed 9: Mo
ves the telescope quickly from one point in the sky to another.
Observe the Moon
Point your telescope at the Moon (note that the Moon is not visible every night) and
practice using the Arrow keys, the digital front focus and the slew speeds to view different features.The Moon contains many interesting features, including craters, mountain ranges, and fault lines. The best time to view the Moon is during its crescent or
half phase. Sunlight strikes the Moon at an angle during these periods and adds a
depth to the vie
w. No shadows are seen during a full Moon, making the overly bright
surface to appear flat and rather uninteresting. Consider the use of a neutral density
Moon filter when observing the Moon. See
SERIES 4000 PHOTO-VISUAL FILTERS, page
48. Not only does it cut down the Moon's bright glare, but it also enhances contrast,
providing a more dramatic image.
Astronomical Observing
Used as an astronomical instrument, your telescope has many optical and electromechanical capabilities. It is in astronomical applications where the high level of optical performance is readily visible.The range of observable astronomical objects is limited only by the observer’s motivation.
To Track an Object Automatically
As the Earth rotates beneath the night sky, the stars appear to move from East to
West. The speed at which the stars move is called the sidereal rate. You can setup
your telescope to move at the sidereal rate so that it automatically tracks (follows) the
stars and other objects in the night sky. If the telescope is not tracking an astronomical object, the object will drift out of the eyepiece field of view. The tracking function
automatically keeps an object centered in the telescope’s eyepiece.
To automatically track objects, you need to learn how the Autostar II keypad operates
in order to move through its menus.You'll need to initialize and align your telescope.
Tip:
When multiple choices are
If abor
ou ma
Y
m a man
or
u options
utostar
y a
w (>).
x to abor
ted,
ollo
y f
le within an A
ailab
v
a
u option, the current
II men
option is usually displayed
first and highlighted b
ight pointing arro
r
Note:
Press any key on the
utostar II handbo
A
the GPS fix.
Autostar II then displays
"Enter Date
prompts to perf
al alt/az alignment (see
page 42) or press MODE
repeatedly until "Select
Item" displays to use the
Autostar II men
."
Moving Through Autostar II’s Menus
The Autostar II database is organized in levels for quick and easy navigation.
JPress ENTER (2, Fig. 2) to go deeper into Autostar II's menu levels.
JPress MODE (3, Fig. 2) to move back toward the top menu level.
JPress the Scroll k
eys (7,Fig. 2) to move up and down through the options avail-
able for each level.
JPress the Arrow keys (5, Fig. 2) to enter characters and digits. The Arrow keys are
also used to move the telescope.
JUse the Number keys to enter digits.
Automatic Alignment Feature
Autostar II offers four methods of altazimuth (alt/az) alignment; this section describes
t
how to initialize and align your telescope using
tion of the other alt/az alignment methods, see pages 42 and 43. For information
about equatorial (polar) alignment, see
w
u-
To prepare your telescope for Automatic Alignment:
1.Tighten the R.A. and Dec. locks (13 and 17, Fig. 1a).
2.Verify that Autostar II is properly connected to your telescope. See
AUTOSTAR II
,
page 17.
3.Flip the telescope power switch to the ON position.
.
The Autostar II screen is activated and a copyright message displays briefly, followed
by a short beep. Then Autostar II takes a few moments to start up the system.
Automatic Alignment. (For a descrip-
APPENDIX A, page 57.)
TO CONNECT
22
Important Note:
Once the telescope is
aligned, only use the Arrow
keys to move the telescope. Once the telescope
has been aligned, do not
loosen the telescope locks
13 and 17, Fig. 1a), or
(
move the base manually,
or alignment will be lost.
Important Note:
If the objects you have
chosen are not in the
eyepiece after after
alignment, it is also
recommended that you
CALIBRA
This menu allows you to
improve your telescope's
pointing accuracy to alignment stars. It calibrates to
correct slight mechanical
misalignment due to
transport, vibration, or
aging. It is recommended
that calibration be
performed once on a new
telescope after the user
initially assembles it.
When this menu is
selected, the telescope
slews to P
then prompts you to center
P
ENTER. Autostar II uses
the position of Polaris to
fine tune the position of
North and also detects
le
telescope.
TE SENSORS
olar
is and to press
olar
or the base of the
el f
v
.
is. Autostar II
Autostar II initializes the Smart Drive if "On" has been previously chosen from
4.
both the R.A. and Dec. PEC menus in the "Setup: Telescope" menu (the very first
time the system is tur
ned on, the Smart Drive feature will not be enabled). Once
"On" is chosen, Autostar remembers the setting until "Off" is chosen again. If "On"
has been selected, the R.A.
and Dec. motors operate briefly and "Initializing:
Smart Drive" displays.
A message displays that warns not to look at the Sun. At the end of this message,
5.
press the key prompted by Autostar II to signify that the message has been read
and understood.
6."Automatic Alignment" displays. Press ENTER.The system now performs the following routines (press any Autostar II key to abort Automatic Alignment) :
Caution: As the telescope performs the following operations, it will swing
and rotate. Keep a safe distance from the telescope.
a.Finds the home position. Moves the telescope to find the "home" position.
When the home position is found, the system knows the limiting positions of
the telescope and can avoid tangling cables and over-rotating the telescope.
b.Detects “level” of the base of the telescope; finds tilt and tip. To detect
level, Autostar II must calculate "level" at three compass points. See FINDING
TRUE LEVEL
Autostar II also determines the positioning (
in the RCX400 INFO box on page 25.
i.e., tilt and tip) of the optical tube.
c.Finds North. Locates magnetic North, then calculates true North. See
FINDING TRUE NORTH, page 25.
d.Attempts a "GPS Fix." The RCX400's GPS receiver attempts to acquire and
sync up with signals from GPS satellites. "Getting GPS Fix" displays. See
GLOBAL POSITIONING SYSTEM in the RCX400 INFO box on page 25.
THE
After performing these operations, Autostar II now knows:
J The telescope's limiting positions
J Where level is for the telescope
J The location of true North
J The observing site's location
J The date and time
e.Star Alignment. Autostar II then chooses two stars to align upon.
"Searching...." displays. When the telescope slews (moves) to the first star for
alignment, it may not appear in the field of view in the eyepiece. If it is not, look
through the viewfinder—in most cases, the star will be visible. Use the Arrow
keys to move the telescope (you can change speed at which the telescope
moves: see
SLEW SPEEDS, page 21 for more information) until the star is vis-
ible and centered in the eyepiece.The alignment star should be easily recognized and be the brightest star in the area of the sky where the telescope is
pointing. Press ENTER. Repeat this procedure for the second star. For more
information about alignment stars, see
.
w
belo
WHICH ONE'S THE ALIGNMENT STAR?
RCX400 TIPS
Which One’s the Alignment Star?
w can
, ho
utostar has chosen an alignment star with which y
If A
you be sure if the star in your eyepiece is really the alignment star?
The rule of thumb is that an alignment star is usually the brightest star in that
orm a GO TO to an alignment star and you're not sure
ou perf
If y
area of the sky
if you have located the alignment star or it isn't in the eyepiece, look through your
viewfinder. When you view an alignment star in the viewfinder, it stands out dramatically from the rest of the stars in that portion of the sky. The viewfinder will
help you locate a star more quickly than the eyepiece, because it has a much
wider field of view than the eyepiece. Using Autostar, set the slew speed to 6 or
higher and use the Arro
your viewfinder has been aligned with the telescope, the alignment star should
now be in the eyepiece. Set the slew speed to 4 or less and center the star in the
eyepiece.
.
ys to center the alignment star in the vie
e
w k
ou are unf
amiliar
wfinder. If
23
Tip:
The GO TO key also
allows you to perform a
spiral search." A spiral
"
search is useful when the
telescope slews to an
object, but that object is
not visible in the eyepiece
after the telescope finishes its search. (This sometimes occurs during an
alignment procedure.)
Press GO TO when the
telescope stops slewing.
The telescope begins to
move in a spiral pattern at
a very slow speed around
the search area. Look
through the eyepiece and
when the object does
become visible, press
MODE to stop the spiral
search. Then use the
Arrow keys to center the
object.
Important Note:
While performing the
automatic tracking procedure, only use the Arrow
keys to move the telescope. Once the telescope has been aligned,
do not loosen the telescope locks (
Fig. 1a), or move the
base manually, or alignment will be lost.
Tip:
To manually enter the
R.A.
nates of an object:
Press and hold MODE for
o seconds or more
tw
R.A. and Dec. coordinates displa
TO. "Object Position" and
a set of coordinates dis-
ys
pla
and Dec. coordinates of
any celestial object using
Number keys. As soon as
the coordinates are
entered, Autostar II slews
the telescope to the coordinates. Note that the telescope must be initial
ized for this procedure to
operate properly.
13 and 17,
di
and Dec.
Then enter the R.A.
.
coor
Press GO
.
y
.
-
-
The
When the procedure is performed correctly, "Alignment Successful" displays.
If Autostar II does not display this message, perform this procedure again.
Note: Alignment stars may change from night to night. All that is required
is for the observer to center the selected stars in the eyepiece when
prompted.
Observe a Star using the Automatic Tracking Feature
w that your telescope has been aligned, you are able to track celestial objects. In
No
this example, the Autostar II Arrow keys are used to find a star, and then Autostar II's
tracking capability automatically keeps the star centered in your telescope's eyepiece.
1.When Automatic Alignment is completed (as described in the previous section),
"Select Item: Object" displays on Autostar II.
2.Select a bright star from one of the Object menus. You may choose any unobstructed, bright star for the purposes of this example. Use the viewfinder (
21, Fig.
1a) to help line up on the star. Use Autostar II's Arrow keys to center the star in
the eyepiece. The tracking motors will then keep the star you have chosen in the
center of the eyepiece.
Go To Saturn
This exercise demonstrates how to select a celestial object, the planet Saturn, for
viewing from Autostar II’s Solar System library. Objects in the eyepiece should maintain their position even though the Earth is rotating beneath the stars. In other words,
the telescope tracks the chosen objects.
Note: Saturn is not visible the entire year; you may need to choose another object from any of Autostar II's many object libraries; however, the procedure, as described below, remains the same.
1 After the telescope is aligned, press Number key "5."
2.“Solar System: Mercury” displays. Keep pressing the Scroll Down key until “Solar
System: Saturn” displays.
3.Press ENTER. “Calculating” displays. Then “Saturn” and a set of coordinates displays. Note that Saturn’s (and other planets’) coordinates change throughout the
year.
4.Press GO TO. “Saturn: Slewing...” displays and the telescope slews until it finds
Saturn.You may need to use the Arrow keys to center Saturn precisely in the eyepiece. Autostar II then automatically moves the telescope so that it "tracks"
n (or whate
Satur
tered in the e
ver other object you may have chosen);
.
epiece
y
i.e.,Satur
n remains cen
Using the Guided Tour
The Guided Tour feature is an easy and fun method of exploring Autostar II's GO TO
2.Press the Scroll Down key twice. “Select Item: Guided Tour” displays.
our: Tonight’s Best” displays. Press ENTER.
Press ENTER.
3.
“Guided
T
Note: If you wish to try out other Guided Tours, press the Scroll Down key
to scroll through other tour choices
, press ENTER.
ys
pla
4.“Tonight’s Best: Searching...” displays. After calculating, “Tonight’s Best: Jupiter”
.
ys
displa
Note: Different objects may be displayed on a tour list on any given night.
Press ENTER to display information about the object. Press GO TO to move the
telescope to the object.
“T
When the tour y
.
ou wish to select dis
-
-
24
Press MODE to return to the Tour list. Press the Scroll keys to scroll through the
5.
list. Press ENTER when you find the next object you wish to observe.
Press and hold down MODE for two seconds to leave the Guided Tour menu.
6.
Other Guided Tours are available, such as "How Far is Far" and "A Star's Life." If you
have programming skills, you may wish to create a custom Guided Tour. See
YOUR OWN GUIDED TOUR, page 63.
CREATE
RCX400 INFO
GPS
Receiv
Fig. 26: RCX400 GPS Receiver.
er
The Global Positioning System
The Global Positioning System (GPS) is comprised of 24 satellites orbiting
the Earth that are constantly transmitting their precise position and time.
The system provides highly accurate, worldwide positioning and navigation
information for any number of applications.
GPS receivers on the Earth acquire signals from three to twelve satellites
to determine the precise latitude, longitude, and time of the receiver.
(Accuracy of the receiver's position may be within 10 to 15 feet.) As
Autostar II uses latitude, longitude, and time information to calculate the
positions of celestial objects, GPS is an ideal tool for aligning your
telescope.
RCX400
Detecting True Level
To detect level of the base of the telescope, Autostar II must calculate the tip
and tilt of the telescope at three compass points and then compensate for it.
Finding level involves the geometric calculations of a "plane." In order to
define a plane, three positions are necessary. This is not unlike building a
table: For a table to stand level and solid, it must have a minimum of three
legs. Autostar II makes gravitational measurements to make a precise determination of true level.
Finding True North
Locating True North is one of the most important ingredients in the alignment
of a telescope. True North is the axis—the pole—which the Earth spins about
and is a key reference for the motion of the Earth.
As you look at the night sky, the stars seem to move; in fact, if you watched
long enough or took a long time-exposure photograph, you'd realize that the
rue North. When
e around one point—the pole or
olv
stars seem to re
Autostar II knows where True North is and also knows the time, it can calculate the location of all the other objects in the sky
One traditional way to find True North is to locate the North Star, Polaris,
which lies very close to True North. Another way to calculate True North is to
use gyroscopes or accelerometers.
The RCX400 determines True North by using a magnetic North sensor. The
sensor locates magnetic North. Magnetic North is not True North, but a
measurement of the magnetic lines of the Earth. Magnetic North may deviate several degrees from True North. But Autostar II, using the observation
site location determined by the GPS and magnetic North information, can
calculate the position of
Some areas are subject to magnetic disturbances, and the magnetic field of
the Earth changes slightly from year to year. Autostar II allows you to adjust
for discrepancies in the local magnetic field using the "Calibrate Sensors"
option in the
v
elescope men
T
.
th.
ue Nor
r
T
See page 34 for more information.
u.
T
25
Select Item:
Setup
Select Item:
Utilities
Select Item:
Glossary
Select Item:
Guided Tour
Select Item:
E
vent
SETUP MENU
A
utomatic alignment
permits all telescope
ope
rations with only
minimal setup.
UTILITIES MENU
Calculate
eyepiece
magnifications;
set timer ale
rts;
create your own
landma
rk survey.
GLOSSARY
What is an elliptical galaxy?
H
ow far away is the Sun?
Expand your knowledge of
astrono
my by displaying terms
and definitions, and other information.
OBJECT MENU
W
ant to see Mars? The Orion nebula?
The Andromeda galaxy? Select from
over 180,000 objects and press
GO
TO to move the telescope
automatically to an object.
EVENT MENU
Display the time of
past, present, and future
astronomical events,
such as Moon phases
or meteor sh
owers.
GUIDED TOUR
A
utostar II escorts you
on a tour of tonight's
best celestial objects
at your viewing location.
Date
Time
Daylight Saving
Telescope
Targets
etc.
Setup
Align
Fig. 28: Menus set in a loop.
26
Fig. 29: Menu options display on the
second line
move up or down through the list of
options
desired option.
Use the Scroll k
.
. Press ENTER to select the
e
ys to
BASIC AUTOSTAR II
Fig. 27: The Autostar II Universe: The six primary categories listed in the Select Item menu
of Autostar II.
It is important to understand that menu selections are set in a loop (Fig. 28).This means
that pressing the Scroll Down key (
options within a given category, then returns to the first option. The Scroll Up key (7, Fig.
2) cycles up through the options in the opposite order. Note that this capability is a quick
way to get to an option that is near the bottom of the list.The following example demonstrates this capability.
Example:
To navigate to the “Select Item: Setup” menu option when the “Select Item: Object”
menu is displayed:
1.Press the Scroll Down key five times or the Scroll Up key once.
The screen in
menu. The second line displays an option which may be selected within that menu.
Some options are choices that select the next menu level down. The Scroll keys move
up and down within the list of available options, showing one option at a time.
When the desired option is displa
choose that option and move down one menu level.
Press the MODE key to leave a menu level;
Autostar II Navigation Exercise
To demonstrate how the Autostar II menu structure works, the following exercise calculates Sunset time so an evening observing session can be planned.
To Calculate Sunset time:
1.Press the MODE key several times, until “Select Item: Object” is displayed.
2.Press the Scroll Down key once to display the “Event” option in the “Select Item”
men
Press the ENTER k
3.
"Event: Sunrise" is displayed.
Fig.29displa
Important Note: No matter how many levels into Autostar II are traveled,
each press of the MODE key moves up a level, until the top level, "Select
Item," is reached. Once in the Select Item level, press MODE to return to
the topmost level, "Select Item: Object."
u.
7, Fig. 2) cycles down through all the available
ys two lines of information. The top line shows the current
yed on the second line, press the ENTER key to
e.g., the wrong menu option is chosen.
ey to choose the "Event" option and move down a level.
Display
MODE
ENTER
Arrow
keys
Scroll
Up
Fig. 30: Some of the features of the
Autostar II handbox.
Tip:
Scroll
Down
When multiple choices
are available within a
menu option, the current
option is usually displayed first and highlighted by a right pointing
arrow (>).
4.Press the Scroll Down key once to display the "Sunset" option in the Event menu.
Press the ENTER key to choose the "Sunset" option and move down another
5.
level.
6.Autostar II calculates the Sunset time based on the current date, time, and loca-
Autostar II then displays the results of the calculation.
tion.
7.Press MODE once to start moving back up through the Autostar II levels. The first
vel up is the Event menu.
le
8.Press MODE again to move up another level. This is the top level, "Select Item."
9.Press MODE again to return to the starting point of "Select Item: Object."
Example of Locating a menu
As you typically will be using menus after you initialize and align your telescope, this example
will assume you have just completed aligning your scope. AutoStar II displays “Select Item:
Object” after the alignment procedure; this will be our starting point. In this example, we will
locate the “Owner Info” option. See
example.
1.“Select Item: Object” displays.
2.As the Owner Info option is in the Setup menu, you will have to use one of the Scroll keys
to navigate through the list of menus. Press the Scroll Down Key. “Select Item: Event” displays
3.Keep pressing the Scroll Down key. Notice that all the menus display as you press the key:
Guided Tour, Glossary, Utilities, Setup. Stop when “Select Item: Setup” displays. If you press
the Scroll Down key one more time, “Select Item: Object” will display again. This is because
the list of menus or options cycles through each choice over and over again when you press
one of the Scroll keys.
4.With “Select Item: Setup” displayed, press ENTER. Pressing ENTER selects the menu or
option currently displayed.
5.“Setup: Align” displays.
6.Press the Scroll Down key again. “Select Item: Date” displays. Autostar II will now display
all the choices that are available with the Setup menu.
7.Continue to press the Scroll Down key until “Setup: Owner Info” displays.
8.Press ENTER. “Owner Info: Name” displays. Press ENTER again. “Name” displays, with the
second line blank. On this line you may enter your first and last name into Autostar II’s memory.
9.Press the Up or Down Arrow key. Notice that a letter of the alphabet displays. Continue to
press one of the Arrow keys until the first letter of your name displays.
10. Use the Right Arrow key to move to the next position so you can choose the second letter
of your name. Continue to use the Arrow keys to enter your full name.
11. Press ENTER when you are finished. Your name is now entered into AutoStar II’s
memory.
12. “Owner Info: Name” displays again (if you wish, you can press the Scroll Down key—“Owner
Address” will display and you can enter your address if you wish).
o:
Inf
Press MODE and
13.
displays. MODE allows you to backup and exit through the menu structure.
Fig. 30 for the location of the Autostar II keys used in this
Navigating Autostar II
Autostar II's menus are organized for quick and easy navigation:
JPress ENTER to go deeper into Autostar II's menu levels.
JPress MODE to mo
ve back toward the top menu level.
JPress Number key "1" to engage the Speed mode, and then press Number keys
1 through 9 to change speeds.
JPress Number k
y "4" to access the F
e
ocus menu.
JPress Number key "7" to access the Reticle menu.
JPress the Scroll keys to move up and down through the options or lists.
JPress the Arrow keys to move the cursor across the display.
JPress the Help (?) k
y to access on-line help
e
.
27
OTA Fan
Dew Heater
OTA Temperature
Ambient Te mp.
Timer
Set
Start & Stop
Alarm
Set
On & Off
Eyepiece Calc.
Field of View
Magnification
Suggest
Sun Warning
Brightness Adj.
Contrast Adj.
Panel Light
Aux Port Power
Beep
Te mperature
Battery
Landmark Survey
Sleep Scope
Park Scope
Sunrise
Sun Transit
Sunset
Moonrise
Moon Transit
Moonset
Moon Phases
Next Full Moon
Next New Moon
Next 1st Qtr
Next 3rd Qtr
Meteor Showers
Quadrantids
Lyrids
Etc.
Solar Eclipses
Lunar Eclipses
Min. of Algol
Autumn Equinox
Vernal Equinox
Winter Solstice
Summer Solstice
Tour Objects
A...
Accretion Disk
Etc.
B...
C...
Etc.
Align
Automatic
Easy
One Star
Two Star
Align on Home
Date
Time
Daylight Saving
Smart Mount
Configuration
Off
On
Train
Update
Load
Save As
Delete
Erase
Telescope
Mount
Model
Focal Length
Max Slew Rate
Focuser
Collimate
Mount Upper Limit
Mount Lower Limit
Park Position
Calibrate Home
Anti-Backlash
Train Drive
Calibrate Sensors
Tracking Rate
Guiding Rate
Reverse L/R
Reverse Up/Dn
Home Sensors
GPS Alignment
R.A. PEC
Dec. PEC
High Precision
Targets
Astronomical
Terrestrial
Site
Select
Add
Delete
Edit
Owner Info
Clone
Download
Statistics
Reset
Select Item:
Event
Select Item:
Guided Tour
Select Item:
Glossary
Select Item:
Utilities
Select Item:
Setup
Tonight's Best
How Far is Far
Etc.
Solar System
Mercury
Etc.
Moon
Asteroids
Comets
Constellations
Andromeda
Etc.
Deep Sky
Named Object
Galaxies
Nebulae
Planetary Neb.
Etc.
Star
Named
SAO Catalog
Etc.
Satellite
Select
Add
Delete
Edit
User Objects
Select
Add
Delete
Edit
Landmarks
Select
Add
Delete
Identify
Browse
Start Search
Edit Parameters
Select Item:
Object
Moon
Overview
Landing Sites
Apollo 11
Etc.
Craters
Abbot
Etc.
Mountains
Mons Bradley
Etc.
Mare, Lakes
Lacus Aestatis
Etc.
Valley, Rills
Rima Agatharchid
Etc.
Calibrate
GPS-UTC Offset
AUTOSTAR II's MENUS
Hold down MODE for two seconds and the
following data displays:
• Right Ascension and Declination coordinates
• Altitude and Azimuth coordinates
• Local Time and Local Sidereal Time (LST)
• Timer and Alarm Status
• Date
• Site coordinates
• Battery status
Hot Buttons
Press the following keys to display
the corresponding menu:
KeyMenu
1Speed
2Caldwell catalog (C)
3Messier catalog (M)
4Focus
5Solar System (SS)
6Star library
7Reticle (RET)
8Index catalog
9New General catalog (NGC)
ucture.
Tree Str
u
utostar II Men
28
The Complete A
Figure 31:
Want to learn more about
Observing Satellites? See
page 39.
Want to learn more about
Landmarks? See page 39.
Object Menu
Almost all observing with Autostar II is performed using the Object menu category.
(
Note: Exceptions include Guided Tour and Landmark Survey.)See GO TO SATURN,
CREA
USING THE
TING USER
page 24, for an example of observing using the Object menu. Also see
GUIDED TOUR, page 24.
Autostar II contains many libraries of viewable objects, such as stars, planets, comets,
nebulae and so forth. When one of these objects is selected from a library, Autostar II
moves your telescope (if properly aligned) and points it at the selected object. Six of the
most popular libraries can be accessed directly using the hot buttons.
The Object Menu options include:
Solar System: A library of the eight planets (Earth is not included) in order out from
the Sun, followed by the Moon, asteroids, and comets.
Constellation: A library of all 88 Northern and Southern Hemisphere constellations.
When this menu option is chosen and a constellation name appears on the first line
of the screen, press GO TO once to change the second line to the name of the brightest star in the constellation. Press GO TO a second time to slew the telescope to that
star. Use the Scroll keys to cycle through the list of stars in the constellation, from
brightest to dimmest.
Deep Sky: A library of objects outside our Solar System such as nebulae, star clusters, galaxies, and quasars.
Star: A catalog of stars listed in different categories such as named, double, variable,
or nearby. Also included are the Hipparcos, SAO, HD, and HR catalogs. The Star catalog may also be accessed directly by pressing the Number key "6."
Satellite: A library of Earth-orbiting objects such as the International Space Station,
the Hubble Space Telescope, Global Positioning System (GPS) satellites, and geosynchronous orbit satellites.
Catalogs are accessed directly using the Autostar II "hot keys": Caldwell (key
Other
"2"), Messier catalog ("3"), Solar System ("5"), IC ("8"), and NGC ("9").
To slew the telescope to catalog objects:
Enter the catalog number of the object using the Number keys and then press ENTER.
For example: To slew to NGC 6720, press Number Key "9," then using the Number
keys, enter the digits "6-7-2-0." Then press ENTER.
Autostar II displays the common name and alternate names of the object, if available.
Press one of the Scroll keys to display some or all of the following information about
that object: Type of object (galaxy, nebula, etc.), Dec. and R.A. coordinates, constellation it is located within, magnitude
object is a star. If further information is available, it displays as scrolling text.
Press GO TO. The telescope, if aligned (see
slew to that chosen object. Press MODE repeatedly to return to previous menu levels.
User Objects: Allows the user to define and store in memory deep-sky objects of specific interest that are not currently in the A
OBJECTS
Landmarks: Stores the location of terrestrial points of interest in the permanent
Autostar II database. This function works with a telescope that remains in one fixed
spot or can be setup in the exact same spot each time it is used.
JSelect: To select a Landmark already in the database (see ADD below), choose
JAdd: To add a Landmark, choose the "Add" option. Enter a name for the
, page 38, f
the "Select" option and scroll through the list. Press ENTER to select a Landmark,
then press GO TO and the telescope slews to the object.
Landmar
tant Note:To add objects to the Landmar
Impor
must be located and aligned exactly as when the original objects were
added to the database.
or more inf
Locate and center the Landmar
k.
, size, distance, and star-type classification, if the
AUTOMATIC ALIGNMENT, page 22), will
ies. See
ar
, then press ENTER.
epiece
y
k database, the telescope
mation.
or
utostar II libr
k in the e
29
Identify: An exciting feature for an observer who wants to scan the night sky and start
exploring. After the telescope has been properly aligned, use the Autostar II Arrow
keys to move about in the sky. Then follow this procedure:
Important Note: Only use the Arrow keys to move the telescope during
the Identify procedure
. Do not loosen the telescope locks or move the
base or alignment is lost.
1.When a desired object is visible in the eyepiece, keep pressing MODE until the
“Select Item: Object” menu is displayed. Press ENTER to select this menu.
Scroll through the Object menu options until the “Object: Identify” screen appears.
2.
3.Press ENTER. Autostar II searches the libraries for the identity of the object being
ved.
obser
4.If the telescope is not directly on an Autostar II library object, the nearest library
object is located and displayed on the screen. Press GO TO and the telescope
slews to that object.
Want to learn more about
using the Browse menu?
See page 41.
Definition:
Transit is the time when
the Sun, Moon, or other
celestial object crosses an
observer's meridian, i.e.,
the time when an object is
at its highest point in the
sky on any given date.
ARNING!
W
Never use
your Meade
Telescope to look at the
Sun! Looking at or near
the Sun will cause instant
and irreversible damage
to your eye. Eye damage
is often painless, so there
is no warning to the
observer that damage has
occurred until it is too
late. Do not point the telescope or its vie
or near the Sun. Do not
look through the telescope or its vie
it is moving.
should always have adult
supervision while observing.
RCX400
wfinder at
wfinder as
Children
®
Browse: Allows you to search the library for objects with certain parameters, much
like a search engine. "Edit Parameters" lets you set various parameters for the search,
such as: Object Type, Minimum Elevation, Largest,
etc. Once you have set the parameters of the search, select "Start Search" and press ENTER. Autostar II will display the
results of the search.
Event Menu
The Event menu provides access to dates and times of astronomical events. The
Event database includes:
Sunrise, Sun Transit, and Sunset: Calculate the time of Sun rise, Sun transit, or Sun
set on the current date. Find rise and set times for other dates by entering a new date
into the “Setup: Date” menu.
Moonrise, Moon Transit, and Moonset: Calculate the time of Moon rise, Moon tran-
sit, or Moon set on the current date. Find rise and set times for other dates by entering a new date into the “Setup: Date” menu.
Moon Phases: Displays the date and time of the next Full, New, 1st Quarter, and 3rd
Quarter Moon.
Meteor Showers: Provides information
Perseids, the Leonids, etc. Also lists the dates of the showers and when they reach
maximum.
Note: Meteors are fast moving objects that cover large areas of the sky and
are usually best observed with the naked eye.
Solar Eclipse: Lists upcoming Solar Eclipses, including the date and type (total,
annular, or partial) of eclipse. Use the Scroll Up and Down keys to display the available data. Remember, never use a telescope to look at the Sun! See
left.
Lunar Eclipse: Lists upcoming Lunar Eclipses, including the date and type (total, partial, penumbral) of eclipse. Use the Scroll Up and Down keys to display the available data.
Min. (Minimum) of Algol: Displays the minimum brightness of the dramatic eclipsing
binary star system, Algol. It is relatively close at a distance of 100 light years. Every
ing a 10-hour per
ys dur
2.8 da
nitude as one of the tw
o stars thus dips from +2.1 to a minimum of +3.4 halfway through the eclipse as
the tw
iod, Algol undergoes a major change in apparent mag
o stars passes behind the other
the second star is hidden. Autostar II calculates minimum magnitude time at mid-
.
eclipse
Autumn and Vernal Equinox: Calculate the time and date of the fall or spring equinox of the current year.
Winter and Summer Solstice: Calculate the time and date of the winter or summer
solstice of the current year.
on upcoming meteor showers, such as the
WARNING! to the
The combined magnitude of
.
-
30
Glossary Menu
The Glossary menu provides an alphabetical listing of definitions and descriptions for
common astronomical ter
Glossary menu or through hypertext words embedded in Autostar II. A
y word in [
is an
when reading a scrolling message such as a description of a planet or star. Press
ENTER whenever a hypertext word is on screen and Autostar II goes to the glossary
entry for that word.
o access directly from within the Glossary menu, use the Scroll keys to scroll through
T
the alphabet. Press ENTER on the desired letter. Scroll to the desired entry and then
press ENTER to read the description.
brac
ms and Autostar II functions. Access directly through the
hypertext word
kets
], usually f
ound when using the Autostar II Help function or
Utilities Menu
The Utilities menu provides access to several extra features within Autostar II, including a countdown timer and an alarm. The Utilities functions include:
OTA Fan: Allows you to turn the fan off or on. The fan assists with the stabilization of
the optics. The fan should be activated at the beginning of an observing session and
run until the optics have achieved an equilibrium with the environment. Fan operation
time should range from about 5 to 25 minutes. Note that the fan may introduce a slight
vibration and this may cause noticeable movement observed with sensitive optics.
Dew Heater: Allow you to adjust heater level, setting from 0 to 100.
OTA Temperature: Provides a temperature reading at the edge of the corrector plate.
Ambient Temperature: Provides a temperature reading at the fork arm.
Timer: Selects a countdown timer. This feature is useful for functions such as
astrophotography and tracking satellites. To use the Timer, press ENTER, then
choose “Set” or “Start/Stop."
Tip:
The Contr
feature is usually only
required in very cold
weather.
If you adjust the contrast so
that you can no longer
read the display, turn off
the po
again. When Version
appears on the display (the
initial displa
not affected by the
Contrast control), press
MODE.
ast Adjustment
er and tur
w
y screens are
n it on
J
Set: Enter the time to be counted down, in hours, minutes, and seconds, then press
ENTER.
JStart/Stop: Activates the timer set previously. Use the Scroll keys to toggle between
ON and OFF. When ON is displayed, press ENTER to activate the timer. When the
timer runs out, four beeps sound and the timer is deactivated.
Alarm: Selects a time for an alarm signal to sound as a reminder. To use the Alarm,
press ENTER, then choose "Set" or "Start/Stop."
J
Set: Enter the time of day for the alarm to sound, in hours, minutes, and seconds,
then press ENTER.
JStar
Eyepiece Calc: Calculates information about an eyepiece for the specific telescope
to which A
JField of View: Scroll through a list of available eyepieces. When an eyepiece is
JMa
JSug
Sun Warning: Enables or disables Autostar II’s Sun warning display.
Brightness Adj:
plete, press ENTER.
Contrast Adj: Adjusts the contr
press ENTER.
t/Stop:Activ
between ON and OFF. When ON is displayed, press ENTER to activate the
alar
m.
When the alar
ate the alar
v
utostar II is connected.
selected, the field of vie
gnification:
selected, the magnification is calculated.
gest:Autostar II calculates and suggests the best eyepiece for viewing,
based on the telescope and the object being vie
ates the alar
m time arrives, Autostar II beeps. Press ENTER to deacti-
m.
Scroll through a list of a
Adjusts the br
m set pre
w is calculated.
ightness of the displa
ast of the displa
viously
yepieces. When an eyepiece is
le e
ailab
v
ed.
w
y using the Scroll keys. When com-
y using the Scroll k
Use the Scroll k
.
eys to toggle
ys. When complete,
e
31
Want to learn more about
Landmarks? See page 39.
Panel Light:
Aux Port Power:
Beep: Turns the beep alerts on or off.
Temperature: Gives a temperature reading of the ambient air. This reading is not always
available.
Landmark Survey: Automatically slews the telescope to all user-defined landmarks
with a shor
in progress, press any key to skip that object and go to the next landmark on the list.
To observe a landmark for a longer period, press MODE when paused on the object
to stop the survey. Press ENTER to restart the survey at the first object on the list.
Sleep Scope: A power saving option that shuts down Autostar II and the telescope
without forgetting its alignment.With "Sleep Scope" selected, press ENTER to activate
the Sleep function. Autostar II goes dark, but the internal clock keeps running. Press
any key, except ENTER, to re-activate Autostar II and the telescope.
Park Scope: Designed for a telescope that is not moved between observing sessions.
Align the telescope one time, then use this function to park the telescope. The next
time it is powered up, pressing ENTER causes the telescope to move to its predetermined Park position. Once parked, the screen prompts to turn off power.
Allows you to turn off LED panel light.
Allows you turn off and on the 12vDC OUT power port.
t pause at each location. Press ENTER to start the survey. While a slew is
Important Note: When the "Park Scope" option is chosen and the display
prompts you to turn off the telescope's power, Autostar II is unable to be
returned to operation without turning the power off and then back on.
Setup Menu
There are numerous other features available within the Setup menu, including:
Align on Home: For permanently mounted telescopes only. If Calibrate Home has
been performed, power up your telescope and select this menu to return the previously calibrated home position. In other words, the telescope is fully aligned according to the setting that were stored in Autostar II's memory during the Calibrate Home
procedure. See
Date: Changes the date used by Autostar II.This function is useful to check events in
the past or future. For example: Set the Date menu for a day three months in the
future. Then check the "Select Item: Event" menu for the Sunset time on that date. See
EVENT MENU, page 30.
Time: Changes the time entered into Autostar II. Setting the correct time is critical for
Autostar II to proper
or 24-hour mode (military time). To select the 24-hour mode, press ENTER when the
lank" option displa
the "b
ylight Sa
Da
Note: Daylight Savings Time may be referred to by different names in various areas of the w
CALIBRATE HOME, page 33, for more information.
vents. Time may be set to "AM," "PM,"
ylight Sa
vings time setting.
.
ify
er
ving
ly calculate locations and e
ys (
i.e., neither "AM" nor "PM" is displa
Enab
:
les or disab
ld.
or
les the Da
k local time to v
Chec
y
ed).
RCX400 TIPS
Look into the Future
The Autostar II Date option in the Setup menu is much more than just an entry
of today's date; with it you can look far into the future or learn about past
Autostar II can calculate the date and times of future events and, except
.
ents
v
e
or eclipses, past events as well (based on the current calendar system).
f
a Sunrise on March 6, 2043 A.D. or the Vernal Equinox in 1776 A.D.To use this
feature, enter the desired date in the Setup menu or select an option in the
Event menu.
Autostar II, using the Event menu, can calculate dates and times for Sunrises,
Sunsets, Moonrises, Moonsets, Moonphases, Solar and Lunar Eclipses (for
xt 100 y
the ne
mums of Algol.
One very practical use of the Event menu is to check the Sunset option to
determine when you can begin your astronomical observing session.
ears), meteor showers, equinoxes and solstices, and the mini-
E.g.,
32
Smart Mount: See page 69 for detailed information.
GPS-UTC Offset: Univ
GPS does not. The offset is the number of leap seconds added since the establishment of GPS
Telescope: Accesses several options, including:
JMount: Set this option to "Alt/Az" if using alt/az alignment and to "Polar" if using
polar alignment. "Alt/Az" is the default value.
JModel: Allows you to select the telescope model connected to Autostar II.
JFocal Length: Displays the focal length of the selected telescope.
JMax Slew Rate: Sets the upper limit for the slew rate. 8 degrees per second is
the fastest setting.
JFocuser: Allows you to recalibrate your focuser. Normally, not used. Recalibrates
focuser and focuser backlash.
JCollimate: Allows you use the Arrow keys to collimate the telescope. See pages
51 and 52 for more details.
JMount Upper Limit: Allows you enter a number from 0 to 90 that sets an upper
limit as to how far the optical tube can swing upward during a programmed slew.
(Note that it does not prevent you from performing a manual slew past this limit.)
This is useful when you have a camera or other peripheral attached to the telescope—you can prevent it from striking the telescope base. 90 (straight up) is the
maximum value that can be entered.
JMount Lower Limit: Allows you enter a number from 0 to 90 that sets a lower
limit as to how far the optical tube can swing downward during a programmed
slew. (Note that it does not prevent you from performing a manual slew past this
limit.) This is useful when you have a large optical tube (12" model) or have a
dewshield attached to the telescope—you can prevent it from striking the telescope base. -90 (straight down) is the maximum value that can be entered.
JPark Position: For permanently mounted telescopes only. After aligning your tel-
escope, select this menu and power down the telescope. The alignment settings—level, North, time, alignment stars—are stored in Autostar II's memory and
are remembered after you power off the telescope. When you power on the telescope, "Automatic Alignment" displays after the start up routine. Press MODE (do
not press ENTER). The telescope remembers its alignment and you can continue viewing or performing other operations without aligning the telescope again.
Park Position provides two options. Use Current Position uses the last position
set by the user. Use Default Position levels telescope and points it North.
JCalibrate Home: For permanently mounted telescopes only. After aligning your
telescope, select this menu and the alignment settings—level, North, time, alignment stars—are stored in Autostar II's memory and are remembered after you
power off the telescope. You can enable Autostar II to retrieve and automatically
align your telescope using these settings the next time you power up by choosing the Align on Home menu. See
tion.
JAnti-Backlash: This option allows you to change the backlash along either the
R.A. and the Dec.axes by entering a number from 0% to 199%.This sets the backlash in the way the Arrow keys move the telescope along an axis. If you enter a
value near 199%, telescope responds more quickly as you hold down an Arrow
key. If you enter a value near 0%, it takes longer for the tube to respond as you
hold down an Arrow key. Experiment with this option: Try changing the values until
the motion of the telescope (while holding down an Arrow key) feels comfortable
to you.
JTrain Drive: All telescopes have a certain amount of "backlash" (looseness in the
inter
the Altitude and Azimuth motors—which helps locate objects with more precision.
.
Note: This method is not as precise as PARK POSITION (see above).
y of gears).
pla
ersal Time (UTC) adds leap seconds to its time calculations,
ALIGN ON HOME, page 32, for more informa-
This menu allows you to compensate for the backlash in the
33
North
Dec.
Setting
Circle
Level
Base
Fig. 32: Alt/Az Home Position. Note
that the Control Panel should face
South, which is not depicted in the
above photograph.
Fig. 33: Dec. Setting Circle at 0°.
Do you want to learn how to
m the
or
perf
correction procedure?
See
RECTION
Tip:
If the "ENTER to Sync" feature is accessed by mistake
(holding the ENTER k
more than 2 seconds),
press MODE to return to
the previous screen.
Want to learn more about
adding and editing sites?
See page 37.
periodic err
PERIODIC ERROR COR-
, page 44.
or
or
y f
e
JCalibrate Sensors:This men
u allows you to improve your telescope's pointing
accuracy to alignment stars. It calibrates to correct slight mechanical misalignment due to transport, vibration, or aging. It is recommended that calibration be
ormed once on a new telescope after the user initially assembles it.
perf
When this menu is selected, the telescope slews to Polaris. Autostar II then
prompts you to center Polaris and to press ENTER. Autostar II uses the position
of Polaris to fine tune the position of North and also detects level for the base of
the telescope.
JTracking Rate: Changes the speed at which the telescope tracks targets in the
sky.
Sidereal: The default setting for Autostar II; sidereal rate is the standard rate
a.
at which stars move from East to West across the sky due to the rotation of
the Earth.
b.Lunar: Choose this option to properly track the Moon over long observing
sessions.
Custom: Allows entry of user-defined tracking rates.
c.
Note: Custom Tracking Rate allows you to enter values from -999 (stands for
99.9%) to 999 (stand for +99.9%). The lower the number, the slower the rate; the
higher the number the faster the rate. If you enter -999, the telescope will move so
slow as to appear to be stopped. If you enter 999, the telescope will be moving at
approximately twice the tracking rate.
JGuiding Rate: Allows you to change the base slew speed, 1x. Enter a percent-
age of the speed (less than 100%) and press ENTER. This function may be useful in guiding the telescope during CCD and long-exposure photography. See
SLEW SPEEDS, page 21, for more information.
JReverse L/R: Reverses the functions of the Left and Right Arrow keys for con-
trolling the telescope's motion (i.e., the Right key moves the telescope to the left).
JReverse U/D: Reverses the functions of the Up and Down Arrow keys for con-
trolling the telescope's motion (
i.e., the Up key moves the telescope down).
JHome Sensors: Turns off or on the True North and True Level sensors, if pre-
ferred, for Easy, One-Star, and Two-Star alignment. User must then manually level
the telescope, set Dec. circle to 0°, point the optical tube to True North and point
the control panel on the base to South during alignment. The default setting for
this menu is "On." See
Figs. 32 and 33.
JGPS Alignment: Allows three options. Select "Off" if you wish to align the tele-
scope manually (turns off GPS). Select "On" (default setting) if you wish to automatically align your telescope and want the telescope to get the GPS fix when it
is needed during alignment. Select "At Start Up" if you want the telescope to get
a GPS fix when the telescope is powered up.
JDec. PEC: Allows you to perform periodic error correction on the Dec. drive worm
gear. Must be performed with a high-power reticle (eg., 9mm).
JR.A.
PEC:
ws you to perform periodic error correction on the R.A. drive worm
Allo
gear. Must be performed with a high-power reticle (eg., 9mm).
aint celestial
JHigh Precision: If High Precision is tur
object (e.g.
ula or galaxy), Autostar II first slews to a nearby bright star and
, a neb
ned on, when looking f
or a f
displays "ENTER to Sync." Center the star in the eyepiece, then press ENTER.
At that point the telescope has a high precision alignment to that part of the sky
and it then slews to the object that was originally requested.
Targets: Switches between Astronomical targets and Terrestrial targets. If
"Astronomical" is selected, the telescope tracking motor is activated and any object
you observe will remain centered in the eyepiece. If "Terrestrial" is selected, the tracking motor is tur
Site: Site pro
. See
ned off
vides access to several options including:
TRACK AN OBJECT AUTOMATICALLY
O
T
, page 22.
JSelect: Displays the currently selected observing site. Use the Scroll keys to cycle
Table 1: Time Zone Shift.
Calculations are for standard
.
time
to select displays. Use this option when you move to a different geographic
location.
JAdd: Allows you to add new observing sites to the database. Scroll through the list
of Countries/States. Press ENTER when the site you wish to add displays. Then
choose the desired city in the same manner
.
However, when the GPS signal is received, the site is normally selected automatically and the site list is updated automatically
. Use of this option is not necessary
and is included for the convenience of those users who may wish to enter a site
manually.You may edit the name of a site using the Edit option (see below).
JDelete: Deletes a stored site from the database.
JEdit: Edits a selected site, including: the name, latitude, longitude, and time zone.
Time Zone refers to the Greenwich Mean Time (GMT) time zone shift. Users
West of Greenwich, England use “-” hours, East of Greenwich use “+” hours. For
the United States, look up the time zone shift in
Table 1.
Note: Autostar II compensates for daylight savings time, if selected. See
SETUP MENU: DAYLIGHT SAVING, page 32.
Owner Info: Accesses the owner information menu, including:
JName: Users may enter both their first and last names using the Up and Down
Arrow keys to cycle through the alphabet. Use the Right and Left Arrow keys to
move through the text. Press ENTER when the entry is complete.
JAddress: Use the Up and Down Arrow keys to enter your street address, city,
state, and zip code. Press ENTER when the entry is complete.
Clone: Uploads information from one Autostar II handbox to another. Three options
are available:
Note:
The Download function
requires the USB cable supplied with the RCX tele-
. See page 43 for
scope
more information on how to
download.
tant Note:
Impor
If your download fails in the
middle of the download
attempt (e.g., your PC
crashes), turn off the tele-
Turn the telescope
.
scope
k on and as soon the
bac
Autostar II display lights up,
press "999." Then attempt
the download again.
JCatalogs: Sends only user-defined object information, such as new satellite
orbits or comet data to another Autostar II handbox.
JSoftware: Sends only the basic Autostar II software.This is useful if one user has
downloaded a new version of Autostar II software from the Meade website
www.meade.com) and wants to pass this software along to friends.
(
JAll: Everything—user-defined information and Autostar II software—is sent to
another Autostar II.
Download: Transfers information from another Autostar II. During the operation, the
“Downloading Do Not Turn Off” appears.
ning
ar
w
JCatalogs: Receives only user-defined object information, such as new satellite
orbits or comet data to another A
JSoftware: Receiv
wnloaded a ne
has do
(
.meade
www
es only the basic A
w v
.com
) and w
ersion of A
utostar II handbox.
utostar II softw
utostar II softw
ants to pass this softw
are. This is useful if one user
are from the Meade w
.
are along to fr
iends
ebsite
JAll: Everything—user-defined information and Autostar II software—is received
by another Autostar II handbox.
Statistics: Provides basic statistical data about Autostar II, including:
ailable in user-defined object
JCharacter
s Free:Displa
ys ho
uch room is a
w m
v
memory.
JVersion: Displays the current version of the Autostar II software.
JSerial Number: Displays the unit's serial number.
Reset: Completely resets Autostar II. Most values entered into the menus revert to
factory defaults. Autostar II requires initialization again after a Reset before proceeding with observations. See
AUTOMATIC ALIGNMENT, page 22.
35
"Hot Button" Menus
Two menus, six object libraries and two functions can be accessed directly using the
Number k
mode and the Utility light are described earlier in the manual.
Focus Control Menus: Press Number key "4" to select these menus directly from
Autostar II's keypad. Each time you press Focus, the key toggles between focus/focus
speed men
Up or Down Scroll keys to select a focus speed (fast, medium, slow or fine). When
“Focuser: Position” displays, use the Up or Down Arrow keys to achieve fine focus of
the object.
You can toggle the Focus key to display the “Focuser: Preset” menus. The Focuser preset menu allows you to assign nine focus positions. If you “park” the telescope, you can
set your own focus, focus for your observing partners and the focus for your camera
or imager. Other Preset menus allow you to select a focus you have assigned and also
to Sync on a Focus Preset.The Sync on a Focus Preset allows you retrieve focus positions when you
see page 32 for information about parking your telescope.
Reticle Control Menu: Press Number key "7" to select this menu directly from
Autostar II's keypad. "Reticle Control: Set Intensity" displays. Press ENTER. The
Intensity menu allows you to change the intensity of the Reticle Eyepiece Illuminator.
Use the Scroll keys to change the value. As you change the value, look through the
reticle to note how the Intensity changes.
When you have finished adjusting the intensity, press ENTER. Press Number key "7"
again and the Rate menu displays. Press ENTER again. Use the Scroll keys to change
the value of the the rate at which the Reticle Eyepiece blinks. As you change the value,
look through the reticle to note how the Blink Rate changes.
When you have finished adjusting the rate, press ENTER. Next, Press Number key "7"
again and the Duty Cycle menu displays. Press ENTER again. The Duty Cycle menu
controls how long the Reticle Eyepiece Illuminator is on during a blink cycle. Use the
Scroll keys to change the value. As you change the value, look through the reticle to
note how the Duty Cycle changes. When you have decided on a Duty Cycle value,
press ENTER.
To exit the Reticle menu, press MODE once.
Object Catalogs: See page 29 for more information.
eys (commonly referred to as "hot buttons"). The two functions, the Speed
us and the preset control menus. When “Focuser: Fast” displays, press the
do not park your telescope. See page 20 for more information. Also
Note: You may continue to change the values using the Scroll keys (and thus
changing the intensity) until you press ENTER again. This allows you to
experiment with the intensity level until you decide which intensity level works
best for you. This feature operates in the same manner in the Rate and Duty
Cycle menus.
36
Important Note:
The Site information is
stored in the Site menu. If
you move the telescope
more than 5 miles of your
initial observing location,
Autostar II automatically
determines your location
when it gets a GPS Fix,
and adds the new location
to the Site menu.
ADVANCED AUTOSTAR II FEATURES
Before trying out the examples in this section, familiarize yourself with the basic operations of A
that you have a basic knowledge of Autostar II and understand how to scroll to a
desired men
that you have initialized and aligned your telescope.
Adding Observing Sites
If you plan to observe using Autostar II at different geographic locations, you can store
obser
Perform these procedures using the Site options (Add, Select, Delete, Edit) of the
Setup menu.
To Add a Site to the user-defined site list:
In this example, you will choose a city and add it to the database list. You will then
select the site to enable it.
1.Navigate to the "Setup: Site" menu. Press ENTER,
2.Scroll through the options until "Site: Add" displays. Press ENTER.
3.Scroll through the list of countries/states. Press ENTER when the country/state
4.Scroll through the list of cities. Press ENTER when the city you wish to add dis-
5.To choose a site, navigate to "Setup: Select." Press ENTER. Scroll through the
utostar II described earlier in this manual. The following examples assume
u or menu option, and how to enter numbers and text. It also assumes
vation sites in Autostar II's memory to help simplify your telescope setup.
you wish to add displays.
plays. The Site is now added to the database. You may add sites using this
method.
list of sites. When the desired site displays, press ENTER.
To Edit a Site:
In this procedure, you will enter a location that is not available in the Autostar II database by editing data of a nearby site.You will edit the location's name, latitude, longitude, and the time zone shift. You will then select the site to enable it.
You will need to know the latitude and longitude of your location to perform this procedure.
1.Using the Add option, choose a site on the list that is closest to your observing
site and press ENTER so that the site is added to your observing sites list.
Choosing a site already on the list (as opposed to using the "Custom" f
es it easier to edit, as the "Time Zone" v
mak
Scroll to "Site:
2.
The name of the site y
3.
scroll to the site
Using the Arro
4.
our obser
of y
5.Press the Scroll Down key and "Edit: Latitude" displays. Press ENTER.
6.Using the Number Keys, enter the latitude of your observing site and then press
ENTER. "Edit: Latitude" displays again.
7.Press the Scroll Down key and "Edit: Longitude" displays. Press ENTER.
Using the Number K
8.
ENTER.
9.Press the Scroll Down key and "Edit: Time Zone" displays. Press ENTER. (If the
ou chose from the list in step 1 has the same
site y
editing, just press ENTER again to go on to the next step.) "Time Zone" refers to
the Greenwich Time Zone shift. Users West of Greenwich, use "-" hours (one hour
per time zone) and users East of Greenwich use "+" hours. For the United States,
look up the shift in
10. After entering the shift, press ENTER. "Edit Time Zone" displays.
Edit" and press ENTER.
ve just entered to your list displays; if it does not,
, enter the longitude of your observing site and then press
ys
e
Longitude" displays again.
"Edit:
,
ABLE 1
T
page 35.
alue ma
"Edit: Name" displays. Press ENTER.
y not need to be changed.
w reads the name
Time Zone as the site you are
eature)
37
Tip:
Using Autostar II to find
objects not in the libraries:
If you do not wish to navigate
through the menus, a more
direct way to enter coordinates is to press and hold
MODE for two seconds or
more. R.A. and Dec. coordinates display. Press GO TO.
"Object Position" and a set of
coordinates displays. Enter
the R.A. and Dec. coordinates
of any celestial object using
Number k
coordinates currently displa
dinates are entered, Autostar
II slews the telescope to the
coordinates. Note that the
telescope must be aligned
(see page 22).
However, if you wish to store
the coordinates of an object
in memor
described at the right.
ys, overwriting the
e
As soon as the coor-
ed.
y
, use the method
y
11. Press MODE. "Site: Edit" displays.
12. Using the Arrow keys, scroll to "Site: Select." The site you have just edited displays. Press ENTER to select the site.
Creating User Objects
In this procedure, you will enter coordinates of celestial objects that do not appear in
y of the Autostar II libraries.You will enter the object's name and R.A. and Dec. coor-
an
dinates (required information). You may also enter the object's magnitude and size
(optional information).
Although Autostar II contains an extensive database of celestial objects (stars, nebulae, planets, etc.) that you can observe, you may eventually want to view objects that
are not par
object's R.A and Dec. coordinates in the "User: Objects" option of the Object menu
and allows automatic slewing of the telescope to the user-entered coordinates.
In order to use this menu option, you first need to look up the R.A and Dec. coordinates of the object or objects you wish to observe. Check your local library, computer
store
Telescope or Astronomy), to find coordinates of celestial objects. The objects/coordinates you enter become part of your own permanent database, called "User Objects."
To enter coordinates of an object into the "User: Objects" option of the Object
menu:
1.Make sure Autostar II has been initialized and the telescope has been aligned.
2.After the telescope is aligned, "Select Item: Object" displays. (If necessary, use
3."Object: Solar System" displays. Keep pressing the Scroll Up key until "Object:
4."User Object: Select" displays. Press the Scroll Down key once. "User Object:
5."Name" displays on the top line and a blinking cursor on the second line. Use the
6."Right Asc.: 00.00.0" displays. Use the Number keys to enter the digits for the
7."Declination: +00°.00'" displays. Use the Number keys to enter the digits for the
8.Autostar II then prompts you to enter the size of the object. This step is optional.
9.Autostar II then prompts you to enter the magnitude of the object.This step is also
To GO TO a user-entered object:
In this procedure, you will choose an object from the User Object list and GO TO the
object.
1.With "User Object: Add" displayed, press the Scroll Up key once. "User Object:
2.
3.
4.Press GO TO and the telescope slews to the object.
t of a library. Autostar II provides a feature that allows you to enter an
, or bookstore for astronomy books, CD Roms, or magazines (such as
Sky &
the Scroll keys to scroll through the menus, as previously described, to find this
option.) Press ENTER.
User Object" displays and press ENTER.
Add" displays. Press ENTER.
Arrow keys, as previously described, to enter the name of the object you wish to
add to the database. When you are finished, press ENTER.
Right Ascension coordinate of your object. When you are finished, press ENTER.
Declination coordinate of your object. If necessary, use the Scroll Keys to change
"+" to "-." When you are finished, press ENTER.
Use the Number keys to enter the size (in arc-minutes), if so desired, and press
ENTER to go to the next display. If you do not wish to enter this information, simply press ENTER.
optional. Use the Number keys to enter this information, if so desired, and press
ENTER to go to the next display. "User Object: Add" displays again.
Select" displays. Press ENTER.
Use the Scroll keys (if necessary) to scroll to the desired object. Press ENTER.
The name of the object and the Right Ascension and Declination coordinates displa
y
.
38
Observing Satellites
In this procedure, you will prepare your telescope to observe a satellite pass.
1. Navigate to the "Object: Satellite" menu option and press ENTER.
2. Use the Scroll keys to scroll through the list of satellites.
3. Select a satellite from the list and press ENTER.
"Calculating...." and then "Tracking..." displays. If the satellite is going to make a
4.
pass, "Located" displays.
5. Use the Scroll keys to display data about the pass: aos—acquisition of signal and
los—loss of signal. If you subtract the aos from the los, you can calculate how
long the satellite will be visible. Location information also displays.
6. "Alarm" displays after the location information. Press ENTER and Autostar II
automatically sets the alarm to sound a minute before the satellite's scheduled
appearance. You may return to regular observations until the alarm goes off.
7. When the alarm goes off, return to the Satellite menu and press a Scroll key until
the desired satellite is on the top line of the display.
8. Press GO TO. Autostar II slews the telescope to where the satellite should
appear. The motor drive stops and a countdown is displayed.
NOTE: If the scheduled appearance position of the satellite is obstructed
(i.e., by a building, tree, or hill), press ENTER and Autostar II starts to
move the telescope along the expected satellite track. When the track
clears the obstruction, press ENTER again to pause the telescope, then
continue with this procedure.
9. With about 20 seconds left on the countdown timer, start watching through the
telescope viewfinder for the satellite to enter the field of view.
10. When the satellite enters the viewfinder field of view, press ENTER. The telescope starts to track with the satellite.
11. Use the Autostar II Arrow keys to center the object in the viewfinder, then look
through the eyepiece to view the object.
Satellite orbits change and new satellites (including the Space Shuttle) are launched.
Visit the Meade website (
updated information and instructions on how to download this data to Autostar II. If
orbital parameters are more than one month old, the satellite pass may not happen at
the time predicted b
your telescope.
Note: Satellite observing is an exciting challenge. Most satellites are in
low orbit, travelling at approximately 17,500 mph. When visible, they move
quickly across the sky and are only in the field of view for a few minutes,
requiring Autostar II to slew the telescope rapidly. Best viewing is near
Sunrise or Sunset when the sky is still dark. Viewing in the middle of the
night can be problematic because a satellite may pass overhead, but not
be visible as it is in the Earth's shadow.
www.meade.com) approximately once a month to get
y Autostar II. Downloading requires the USB cable supplied with
Tips:
To use the Landmark function, the telescope must be
located and aligned exactly
as when the landmark(s)
as added to the database.
w
o add objects to the
T
Landmark database
escope must be located and
aligned exactly as when the
original objects w
to the database
, the tel
ere added
.
Landmarks
ou to define and store terrestr
This men
database. First, a landmark needs to be stored in memory using the "Landmark: Add"
option. To view a landmark, use the "Landmark: Select" option. Landmarks may also
be viewed using the "Landmark Survey" option in the Utilities menu.
o Ad
T
In this procedure
-
memory.
1.Note for future reference where the telescope is located and if you have aligned the
2.Display the "Setup: Targets" menu option. Chose "Terrestrial" and press ENTER.
u option allo
d a landmark to the database:
telescope, which alignment method is used.
"Setup: Targets" displays again. Choosing this option turns off tracking for astronomical objects which is not useful f
ws y
ou will store the location of terrestr
, y
or the vie
ial objects in the Landmar
ial landmarks in Autostar II's
wing of terrestr
ial objects such as
k
39
those in the Landmar
"Astronomical" when you wish to view celestial objects again.
3.Press MODE once. "Select Item: Setup" displays.
4.Press the Scroll Down key once and "Select Item: Object" displays. Press
ENTER. "Object: Solar System" displays.
5.Press the Scroll Up key twice and "Object: Landmarks" displays. Press ENTER.
"Landmark: Select" displays.
6.Press the Scroll Down key once. "Landmark: Add" displays. Press ENTER.
"Landmark Name" displays. Using Arrow keys, enter a name for the landmark you
7.
wish to add to the database. When finished, press ENTER.
8."Center Landmark. Press Enter" displays. Using only the Arrow keys (do not manually move the telescope), move the telescope to the desired landmark and center the object in the eyepiece. Press ENTER. The object is now stored in memory.
9."Landmark: Add" displays. If you wish to add more landmarks, repeat steps 5
through 8.
To Select a landmark from the database:
1.Make sure the telescope is located and aligned exactly as when the desired landmark was entered into memory.
2.Display the "Landmark: Select" menu option. Press ENTER.
3.Use the Scroll keys to scroll through the list of objects you have previously
entered. When the desired object displays, press ENTER to select the object.
k database. Be sure to change this option back to
Use the Scroll keys to scroll through location information about the object, if
desired. Press GO TO to slew the telescope to the landmark.
4.Press MODE to exit.
To perform a Landmark Survey:
This procedure allows you to perform a tour of the objects entered in the "Object:
Landmark" menu option—note that the Landmark Survey will function only if you have
previously entered objects in the Landmark menu.
1.Navigate to "Utilities: Landmark Survey" menu and press ENTER.
2."Landmark Survey: Slewing..." displays. The telescope moves to the first object
on the Survey list and displays the name of the object.
3.Press MODE to stop the Survey. Press ENTER to restart the survey at the first
object of the survey.
le amount of memory in Autostar II:
ailab
k on the a
hec
o c
T
utostar II has a limited amount of memor
A
objects and other bits of information in Autostar II, you will begin to use up memory.
This procedure allows you to check on how much memory is still available.
1.Navigate to the "Setup: Statistics" menu option and press ENTER.
2."Statistics: 37.2K Char. Free" displays. This is the amount of memory that is still
available to the user.
v
. Once you begin to store Landmarks, user
y
Identify
This procedure allows you to use Autostar II to identify objects you have found in the
night sky using the Arrow keys. If the object is not in Autostar II's database, Autostar
II displa
quer
ys inf
ied about.
Impor
tialize and align Autostar II. If you physically move the telescope after initialization, this function will fail to operate properly.
mation about an object in its database that is closest to the one y
or
ou must first ini-
, y
tant Note:For this function to oper
ate proper
ly
ou
40
In this procedure
the telescope eyepiece and use the "Identify" menu to find out information about the
object or the nearest object to it in the Autostar II database.
1.Center the object you wish to have identified in the telescope's eyepiece.
2.Navigate to the "Object: Identify" option and press ENTER.
"Searching..." displays. When Autostar II finishes calculating, the name of the
3.
closest object displays.
4.Press a Scroll key to display information about this object. Autostar II displays
some or all of the f
Scroll key:
Displayed information:Example:
Catalog or common name of objectMessier 107, NGC6171, Orion Nebula, etc
Type of objectGlobular Cluster, Nebula, Black Hole, etc.
Right Ascension16:32:4
Declination13°03'
Constellation
Magnitude3
Size2'
Scrolling message"This Globular Cluster is 10,000 light years
, you will center an object you wish to have identified by Autostar II in
ollowing information about the object with each press of a
Virgo, Orion, etc.
away...."
Browse
This menu allows you to search the libraries for objects with certain parameters, much
like a search engine. "Edit Parameters" lets you set various parameters for the search,
and "Start Search" activates the search. A typical search might be performed as follows:
1.Select "Browse" from the Object menu. Press ENTER. "Browse: Start Search"
displays.
2.Press one of the Scroll Keys and "Browse: Edit Parameters" displays. Press
ENTER.
3."Edit Parameters: Largest (mins)" displays. "Mins" stands for arc-minutes. Press
ENTER.
4."Largest (mins)" and a value displays. Using the Number keys, enter a size in arcminutes. Autostar II will search for objects
ENTER
5."Edit Parameters: Largest (mins)" displays again. Press the Scroll Down key. "Edit
Parameters: Smallest (mins)" displays. Enter the value for the smallest size of an
object that Autostar II will search for in the database. Continue with "Brightest,"
Faintest," and "Minimum Elevation," using the procedure described in steps 3 and
4.
6.After "Minimum Elevation," "Object Type" displays. Press ENTER." "+Black Hole"
displays. If you do
and the "+" changes to a "–." Press the Scroll Down key to scroll to the next item.
"+Diffuse Nebula" displays. Continue to scroll through the list and press ENTER
if you wish to change the "+" to a "–" or vice-versa.
7.After you have scrolled to the last item on the "Object Type" list, press MODE
twice and the Scroll Down key once. "Browse: Start Search" displays. Press
ENTER. "Start Search: Next" displays. Press ENTER. Autostar II searches the
database and displays the first object that matches the search parameters you
ha
MODE and "Star
matching the par
objects
Press MODE repeatedly to lea
8.
.
not wish to have "Black Holes" in your search, press ENTER
ve entered. Use the scroll keys to display information about the object. Press
xt" displa
t Search:
ameters displa
Press GO TO to slew telescope to a displayed object.
.
Ne
.
ys
e this men
v
up to this size and no larger. Press
ys again.
Repeat this procedure to display all the
Press ENTER and the ne
u.
xt item
41
Important Note:
If you disable the automatic
alignment/GPS function and
then use the alternate alignments described in this section, you will be prompted to
enter the Time, Date, and
Daylight Savings status.
Alternate Alt/Az Alignments
If you would rather set up your telescope without using automatic alignment, Autostar
II offers alternative alignment methods for both alt/az and equatorial mounting. During
the One-Star and
and Easy alignment procedures) manually place the telescope in the home position.
The procedures for equatorial (polar) alignment are discussed in
57; the three alternative alt/az alignment methods are discussed below.
Two-Star alt/az alignment procedures, you will (unlike the Automatic
APPENDIX A, page
Initialize Autostar II
First, you need to initialize Autostar II.
1. Tighten the R.A. and Dec. locks (
2. Verify that Autostar II is properly connected to your telescope. See
AUTOSTAR II,
3. Flip the telescope power switch to the ON position.
The Autostar II screen is activated and a copyright message displays briefly, followed
by a short beep. Autostar II takes a few moments to start up the system.
4. A message then displays that warns not to look at the Sun. At the end of this message, press the key prompted by Autostar II to signify that the message has been
read and understood.
6. Autostar II displays "Align: Automatic."
You are now ready to align your telescope using one of the three alt/az alignment procedures.
page 17.
13 and 17, Fig. 1a) to a firm feel.
TO CONNECT
Easy (Two-Star) Alignment
In this method, Autostar II automatically picks two stars from its libraries for alignment.
During the procedure, Autostar II slews the telescope to a first alignment star.The user
is asked to verify that the telescope is pointed at the chosen star and then prompted
to center the star in the eyepiece. The process is repeated with a second star to complete the alignment.
Note: Before performing this procedure, first verify that INITIALIZE
AUTOSTAR II
, above, has been performed.
How to perform the Easy Align Procedure
1.Alignment Option Screen. Following initialization, "Align: Automatic" displays.
2.Select Alignment. Press the Scroll keys until "Align: Easy" displays. Press
ENTER.
Home Position. The telescope automatically sets the following positions: home,
3.
level, North, and True North. You may turn off the sensors and manually set these
positions. See
. Star Alignment. Autostar II chooses two stars to align upon. The telescope slews
4
to the first star for alignment. Should the alignment star not appear in the field of
view in the eyepiece, it should be easily recognized: It will be the brightest star in
the area of the sky where the telescope is pointing. Use the Arrow keys to move
the telescope until the star is visible and centered in the eyepiece. Press ENTER.
Repeat the procedure for the second alignment star.
Note: See WHICH ONE'S THE ALIGNMENT STAR, page 23, for some impor-
tant tips concerning alignments stars and using your viewfinder.
When the procedure is performed correctly, "Alignment Successful" displays. If
Autostar II does not display this message, perform this procedure again. (Keep
pressing MODE until "Align: Easy" displays and repeat the procedure.)
HOME SENSORS, page 34 for more information.
Two-Star Alt/Az Alignment
Two-Star Alignment requires some knowledge of the night sky. Autostar II provides a
library of bright stars and two stars from this library are chosen by the observer for
el, or
v
utostar II does not automatically find home
alignment.
Nor
1.
2.
In this procedure
th.
Alignment Option Screen.
Select Alignment. Press the Scroll keys until "Align: Two Star" displays. Press
ENTER.
, A
"Align:
utomatic" displa
A
ys
.
, le
42
Note:
Autostar II locates alignment stars based on the
date, time, and location
entered. The alignment
stars may change from
night to night. All that is
required is for the observer
to center the selected stars
in the eyepiece when
prompted.
Tip:
Try a Spiral Search
The GO TO key also allows
you to perform a "spiral
search." A spiral search is
useful when the telescope
slews to an object, but that
object is not visible in the
eyepiece after the telescope finishes its search.
(This sometimes occurs
during an alignment procedure.) Press GO TO when
the slew is finished and the
telescope starts slewing in
a spiral pattern at a very
slow speed around the
search area. Look through
the eyepiece and when the
object does become visible,
press MODE to stop the
al search.
spir
Arrow keys to center the
object.
Then use the
3.Set Home P
osition.Place the telescope in the home position.
To Set the Home Position Manually:
a. See Figs. 32 and 33, page 34. Loosen the telescope’s Dec. lock (17, Fig.
). Set the optical tube to 0° on the Dec. setting circle (Fig. 33).
1a
b. Tighten the Dec. lock (
Level the tripod base.
c.
d. Move the base of the telescope so that the computer control panel (
) approximately faces South.
1a
e. Unlock the R.A. lock (
ontally until it points North.
iz
. Re-lock the R.A. lock (
f
17, Fig. 1a) to a firm feel only.
12, Fig.
13, Fig. 1a) and turn the telescope's optical tube hor-
Fig. 1a).Press ENTER.
13,
g. Press ENTER.
4
. Star Alignment. "Select Star" displays. Autostar II then displays a library of stars
for the observer to choose from. Use the Scroll keys to scroll to a star on the list
that you wish to align upon. Select a star that you can easily locate in the night
sky. Press ENTER.
Center Star. The telescope slews to the star. Use the Arrow keys to move the tel-
5.
escope until the star is centered in the eyepiece. Press ENTER.
Center Star. Repeat procedure for the second alignment star. The telescope is
6.
aligned and you are now ready to use Autostar II's GO TO capabilities for a night
of observing.
One-Star Alt/Az Alignment
One-Star Alignment requires some knowledge of the night sky. Autostar II provides a
library of bright stars. One-Star Alignment is identical to Two-Star Alt/Az: Alignment
TWO-STAR ALT/AZ ALIGNMENT, page 42), except only one star from the data-
(see
base is chosen by the observer for alignment.
To Download the Latest Version of Autostar II Software
Included with your telescope is a CD ROM and a USB cable.You need to install the
USB drivers, that are included on the CD ROM, BEFORE plugging in the cable:
1 Select RCX Users (the fourth selection on the list) from the CD Rom.
2 Follow on screen instructions (click “Next” and “Finish” buttons when asked to
do so).
3 Plug in the USB cable. Plug one end into one of the RCX400 USB ports on a
computer control panel/ Plug the other end into a USB port of your PC.
Next, you will install the Autostar Suite software from the CD ROM. This software
provides a menu that allows you to download the latest version of Autostar II
software into the Autostar II handbox.
.
Select A
4.
F
Once the A
5.
utostar Suite on the CD R
w the on-screen instr
ollo
icon on the desktop
uctions
utostar Suite softw
.
OM to install A
.
are installs
, doub
utostar Suite onto y
le-clic
k the ne
w
6.Go to the Telescope menu and select “Update Autostar.” The “Autostar Update”
screen displa
ys
rade Autostar Software Now” button.
“Upg
k the
Clic
.
7.The application detects your telescope type and the version of Autostar software on your handbox.
8.A window displays asking if you wish to download the latest version of Autostar
from your hard drive (if you previously downloaded it separately from the
Select one of the choices and f
Meade w
ebsite) or from the inter
on-screen instr
uctions
.
net.
9.The download will take several minutes (download time depends on your inter-
When the do
th).
net connection, speed of y
complete
, the ne
w version of the Autostar software displays.
our computer and so f
or
our PC
utostar Suite”
“A
w
ollo
wnload is
43
Periodic Error Correction
If you wish to perform high-precision astrophotography, you may wish to "train" your
telescope in order to keep objects that you are imaging dead center in the telescope's
field of view during the photographic exposure. Periodic error correction (PEC) helps
to remove the slight perturbations from center that occur due to the mechanical
nature of a telescope. To perform this procedure, you need to use a high-power reticle, such as the 9mm reticle (see
training is available for both drives.
Train Menu Option
If you perform this procedure in alt/az alignment, you can train the telescope in both
the R.A. and the Dec. axes; in polar alignment, you need only train the telescope's
R.A. axis. If you train the telescope in polar alignment, make sure that "Polar" is
selected in the "Telescope: Mount" menu ("Alt/Az" is the default setting).
To perform the procedure on the Dec. axis (Alt/Az mode), pick a bright star in the East
or West that is about about 20° above the horizon.
To perform the procedure on the R.A. axis (Alt/Az mode), pick a bright star in the
South that has minimal movement and is about 30° above the horizon (
Southern hemisphere, pick a star in the North that is about 30° above the horizon)
Important Note: The Train option overwrites any previous PEC data.
1. Select "Train" from the Dec. PEC menu (in the "Setup: Telescope" menu) and press
ENTER.
2. Look through the reticle. Use the Arrow keys to keep the star centered in the reticle
cross-hairs. Autostar II displays a count of the 200 positions of the worm gear. When
the count reaches 200, one cycle is complete. A full cycle takes about 8 minutes.
3. Select "Train" from the R.A. PEC menu (in the "Setup: Telescope" menu) and press
ENTER.
4. Look through the reticle. Use the Arrow keys to keep the star centered in the reticle
cross-hairs. Autostar II displays a count of the 200 positions of the worm gear. When
the count reaches 200, one cycle is complete. A full cycle takes about 8 minutes.
5. Press MODE to exit.
Update Menu Option
Use the Update option to further refine your training; it is recommended that you
update your original training two or three times when first using your telescope.
Update does not overwrite the data, but updates the training using information gathered from both the last and the current training sessions. Press the MODE key to exit
from this option. If you wish to further refine your training, select this menu again and
repeat the procedure.
Erase Men
Select this option to erase all PEC training data.
On and Off Menu Options
Select "On" when you want the telescope to use the training information. Select "Off"
when you do not want for the telescope to use the training information. Select "On" to
enable the Smart Drive.
u Option
OPTIONAL ACCESSORIES, pages 48 - 50). PEC
Note: If in the
.
44
Fig. 34: Example of vignetting.
PHOTOGRAPHY
The RCX400 optical design consists of a h
mary combination that performs as one hyperbolic element. The corrector plate advantage, aside from the obvious optical correction that the lens produces, allow astrophotographers to make images free of diffraction spikes, with diffraction spikes being the only
real negative to a traditional Ritchey-Chrétien design.
ou may perform through-the-telescope photography with any 35mm camera body with
Y
a removable lens.You may connect a camera to a #62 T-Adapter. Using this method, the
telescope effectively becomes the lens of the camera.
The #62 T-Adapter connects to a T-Mount for the particular brand of 35mm camera
being used, followed by the camera body.
To orient an object in the viewfinder of the 35mm camera body, use a small jeweler’s
screwdriver to slightly loosen three adjustment screws around the outer knurled ring
of the T-Mount. Rotate the camera body to achieve proper orientation of the object;
then re-tighten the adjustment screws.
The #62 T-Adapter permits close-coupling of a camera body to the telescope. In this
ormat vignetting occurs: The photographic image appears on film with a slight dark-
f
ening (vignetting) at the corners of the 35mm frame (
Photography through a long lens such as the RCX400 requires special technique for
good results, and the photographer should probably expect to waste a roll or two of
film in acquiring this technique. Long-lens photography has its own rewards, however,
rewards that short-focus lenses cannot duplicate.
A few tips on photography with the RCX400 telescopes:
1.Use the Field Tripod for the telescope. At an effective focal length of 2000mm or
more, even small external vibrations can easily ruin an otherwise good photo.
For best results in photographing celestial objects, a wedge and One-Star polar
alignment is recommended. See
2.Use a cable-operated shutter release. Touching the camera body to initiate shutter operation almost certainly introduces undesirable vibrations.
3.Focus the image with extreme care. While observing the subject through the camera’s reflex viewfinder, focus the telescope. Note that some 35mm cameras may
have an optional focusing screen (available from the manufacturer) for use with a
long telephoto lens. This screen provides a brighter and clearer image to focus,
and is highly recommended.
4.Correct shutter speeds vary widely, depending on lighting conditions and film
used. Trial-and-error is the best way to determine proper shutter speed in any
given application.
Note: The camera used with your telescope may have an exposure meter
that is still active when the standard lens is removed and the body is connected to the telescope with the T-Mount. If used for terrestrial photography, the camera meter should be acceptable. If used for astrophotography,
the meter probab
not made to compensate for a dark sky.
ly will not pro
yperbolic secondary and corrector lens/pri-
Fig. 34).
APPENDIX A, page 57.
vide good results since camer
a meters are
aphy through the
ial photog
errestr
T
5.
s surface. Long distance photography is best accomplished in the early
th’
the Ear
morning hours before the Earth has had time to build up heat.
aphy of the Moon and planets through the
r
Photog
6.
ifying, but points 1 through 4 should be particularly noted in this case. If you wish
to take photographs using polar alignment, see
r
RCX400 is sensitiv
e to heat w
RCX400 can be especially g
APPENDIX A, page 57.
es r
v
a
ising from
at
r
-
45
35:
Fig.
The Lunar Planetar
y Imager
Photograph
Although digital camer
tional 35mm cameras, they provide some significant advantages to the casual
astrophotographer: You do not have to develop the images (instant images), lower
costs, computer and internet readiness. And because unwanted photos are easily discarded, they provide the freedom to experiment.
Digital cameras present some problems for the astrophotographer: Many models have
lenses that cannot be removed, difficulties in attaching to a telescope, possible
vignetting, lack manual focusing and shorter exposure times.
Shorter exposure times is one of the biggest drawback. Long exposures with digital
cameras introduce undesirable noise and artifacts into a digital image. This limits the
ange of astro images to the Moon, planets and bright stars.
r
Some tips for better photos:
• If you cannot remove the lens to your camera, look for a commercially available
digital T-adapter. New solutions for attaching a digital camera to a telescope are
becoming available as time goes by.
• If the camera is not directly coupled to the eyepiece, keep it as close to the eyepiece as possible and center the image to be photographed to minimize vignetting
(darkening of the edges of the photo).
• Try to block ambient light (from street lights, house, etc.) from the eyepiece and
the camera with a piece of cardboard, a screen, etc.
• Keep extra (charged) batteries on hand for your camera as digital cameras often
drain batteries in a short period of time. Rechargeable Lithium batteries provide
power for a longer period than non-rechargeable batteries. If practical, use an AC
adapter.
• Avoid short-focus eyepieces. They present many difficulties for digital cameras.
• If using manual focus, set to infinity. Otherwise, using the camera's autofocus is
OK.
• Experiment with your camera's exposure, brightness and /or contrast settings.
Keep notes for future reference.
• Clean eyepieces and camera lens as needed.
• Many digital cameras have a manual ISO setting. Short exposures times work the
best.
• Use your camera's highest image quality and lowest compression settings.
Although this fills up your camera's memory more quickly, it produces the best
quality photos
Use the camer
•
.
minimize vibration. Wireless shutter releases may be available for some model
digital cameras. If you do not have a shutter release, use the camera’s timer
(sometimes called “self-timer”), which is available with most digital cameras. The
timer may also minimize vibration.
y with a Digital Camera
as still cannot match the quality of images provided by tradi-
.
a's timer or remote shutter release (if available for your camera) to
Fig. 36: The Deep Sky Imager.
46
Photography with Meade’s AutoStar Suite™
The AutoStar Suite with Meade LPI™ (Lunar Planetary Imager) or Meade Deep Sky
™ turns your Meade RCX400 telescope, AutoStar and PC into even more pow-
Imager
erful and easy-to-use astronomical instrument.
LPI (
Fig. 35) and Deep Sky Imager (Fig. 36) combine the power of an electronic astro-
nomical imager with the simplicity of a web cam. Check out the following imager features:
• Achieve great results the first time out on the Moon, planets, brighter deep-sky
objects and terrestrial targets.
• Easy to use with real-time display of object on your PC screen. Just center, focus
and shoot.
Magic Eye software-assisted focusing.
•
• Automatic and manual exposure control from .001 to 15 seconds (up to 450x
longer than web cams).
Automatically takes multiple exposures.
•
The AutoStar Suite Software includes powerful tools to help you get the most from
your Meade RCX400 telescope:
• Sophisticated planetarium program with over 19 million objects.
• Select objects from the planetarium display and the telescope slews to those
objects.
Create time-lapse movies of objects, such as Jupiter
•
• Create your own Guided Tours.
• Advanced Image Processing Software including Unsharp Masking, Convolution
Filtering and many other features.
• Control all AutoStar functions from your PC.
• Talking Telescope software translates AutoStar text to synthesized speech
through PC speaker.
Includes a cable to connect your RCX model to your PC.
•
See the CD Rom that is included with AutoStar Suite for more information and instruction manual.
Fig. 38a: The Deep Sky Imager
connected to the RCX400
diagonal mirror.
Fig. 37a: Image of M13 captured with
the Deep Sky Imager
Fig. 37b: Image of M51 captured with
the Deep Sky Imager.
.
Fig. 38b: The Deep Sky Imager
connected to the RCX400
with a flip mirror optional
accessory.
47
Fig. 39: Series 5000 5 Element
Plossl Eyepieces.
Fig. 40: Series 5000 Super Wide
Angle Eyepieces.
OPTIONAL ACCESSORIES
A wide assortment of professional Meade accessories is available for the RCX400 tel-
escope models. The premium quality of these accessories is well-suited to the quality
of the instr
An advanced 4-element design flattens the field of view,
er the maxim
um light transmission, the highest contrast and an image free of color fringing. Maintains a comfortable eye relief of longer
focal length eyepieces, while increasing magnification.
Magnification
2x
3x1.254
5x1.254
2x
Series 4000 8 - 24mm Zoom Ey
Barrel Size# of elements
1.25”
2.00 (w/1.25”
epiece:
adapter)
The inter
4
4
oom optics of this e
nal z
yepiece
move on smooth, precisely machined surfaces which maintain optical collimation at
ocal length in
aduated in 1mm units indicates the z
A scale g
oom settings
all z
-
operation. An excellent addition to any eyepiece set.
.
r
oom f
Series 4000 Photo-Visual Color Filters: Color filters significantly enhance visual
and photographic image contrast of the Moon and planets. Each filter threads into the
barrel of any Meade 1.25" eyepiece, and into the barrels of virtually all other eyepiece
brands as well. Meade filters are available in 12 colors for lunar and planetary applications, and in Neutral Density as a lunar glare-reduction filter.
Fig. 43: Series 4000 8 - 24mm Zoom
Eyepiece.
Fig. 44: #905 Variable Polarizer and
#1A Skylight Filter.
Series 4000 Nebular Filters: A modern boon to the city-dwelling deep-space
observer, the interference nebular filter effectively cancels out the effects of most
urban light pollution, while leaving the light of deep-space nebular emissions virtually unattenuated. Meade
technology
the rear cells of Meade Schmidt-Cassegrain models.
Variable Tele-Extender: For eyepiece-projection photography of the Moon and the
planets, a Tele-Extender is required. The Variable Tele-Extender threads onto the
telescope's eyepiece-holder, into which is inserted an eyepiece of typically about
26mm focal length; the 35mm camera body couples to the tele-extender by means of
a T-Mount. The Meade
#928 45° Erect-Image Diagonal Prism: Diagonal mirrors and prisms result in images
that are correctly oriented up-and-down but reversed left-for-right. For terrestrial
observing a fully correctly oriented telescopic image is desirable; the
Prism accomplishes this image correction and places the eyepiece at a convenient
45° viewing angle. The #928 is for use with the 1.25" Eyepiece-Holder.
Series 4000 Plössl 9mm Illuminated Reticle Eyepiece: The most advanced commercially-available illuminated reticle eyepiece, the
powered by an internal battery, includes micrometric x-y positioning controls which
greatly facilitate locking onto the guide star: Turn the finely-threaded controls and
place the reticle’s crossline pattern precisely at the desired position in the field. The
sharp, high-power imaging of the 4-element, multi-coated Plössl optical system is
complemented by a rubber eyecup (foldable for eyeglass wearers) that shuts out distracting stray light from the observer’s eye. The upper (lens) section of the eyepiece
rotates on a fine thread for precise diopter adjustment to the user’s eye. Reticle pattern is a double crossline with two concentric circles.
, and are available with threaded cells for eyepieces or for attachment to
Series 4000 Nebular Filters utilize the very latest in coating
Variable Tele-Extender permits a range of projection images.
#928 Diagonal
Series 4000 Plössl 9mm model,
Fig. 45: Illuminated Reticle Eyepiece.
Fig. 46: #62 T-Adapter.
#62 T-Adapter: The T-Adapter is the basic means of prime-focus photography through
all Meade Schmidt-Cassegrain models. Thread the T-Adapter on to the rear cell of
your telescope, followed by a T-Mount for your 35mm camera, and the camera body
is rigidly coupled to the telescope.
#777 Off-Axis Guider: The Off-Axis Guider provides a means during long-exposure
astrophotography for the photographer to monitor the tracking of the telescope to
assure that the telescope remains precisely positioned on the object being photographed. Like the T-Adapter, the
telescope but it also causes a small amount of the guidestar’s incoming light to be
diverted at a right angle, where the star’s position can be examined for tracking errors
with an illuminated reticle eyepiece; position corrections can then be effected using
Autostar II.
Piggyback Brackets: Piggyback photography is one of the most popular and easiest
ways to get started in astrophotography. Attach your 35mm camera, with its own
35mm-to-250mm lens, atop your
through the main telescope, wide-field photos of the Milky Way of remarkable detail
and clarity can be taken.
Dew Shields: In moist climates, water particles suspended in the atmosphere may
condense on the front surface of the telescope's correcting plate. This dew formation
may be inhibited to a significant extent by the addition of a dew shield, essentially an
extension tube attaching to the front-cell of the telescope.
#905 Variable Polarizer (1.25"): #1A Skylight Filter: The #905 system includes 2
Polarizer filters mounted in a specially-machined cell, for glare-reduction in observing the Moon. Rotate the thumbscrew at the side of the unit to achieve light transmission between 5% and 25% of its original value. The #905 inserts into the diagonal mirror of the telescope, followed by an eyepiece. The #1A Skylight Filter threads
onto the rear cells of all Meade
telescope from dust.
The filter increases visual and photog
.
filter
helps to penetr
All other rear cell accessories may then be threaded to the #1A
.
e
ate haz
Off-Axis Guider couples the camera body to the
RCX400 in equatorial mode, and guiding the camera
RCX models and effectively seals the interior of the
aphic contr
r
ast, decreases glare
, and
49
#1220 Field De-r
and plugs into an RS232 (Serial) port. Digital data fed from the telescope's microprocessor to the field de-rotater permit precise and continuous update of the de-rotation required to maintain pinpoint star images throughout the field. The effect is that
ven during the longest CCD or photographic exposures, the telescope acts as if it
e
were precisely equatorially mounted.
RCX400.
RCX A
Cigarette Lighter Adapter: Powering the RCX400 telescope by means of an automo-
bile cigarette lighter plug.
#644 Flip Mirror System: Has an X/Y adjustment mechanism for the diagonal mirror
with locks for the precise centering, and multiple rotating adapters for T-thread and
1.25” camera attachment. Accepts 1.25” O.D. eyepieces and has a clear aperture of
22mm. Use with small to medium size chip CCD cameras. See
see image of the Flip Mirror System attached to the rear cell of an
#647 Flip Mirror System: Has an X/Y adjustment mechanism for the diagonal mirror
with locks for the precise centering, and multiple rotating adapters for T-thread and
1.25” camera attachment. Accepts 1.25” O.D. and 2.00” eyepieces and has a clear
aperture of 40mm. Use with medium to large size chip CCD cameras. See
page 49, to see image of the Flip Mirror System attached to the rear cell of an RCX400
model.
CCD Framing Ocular: Displays rectangular frame of all popular CCD chip sizes.
Inserts directly into the eyepiece holder or flip mirror. Includes variable LED illumination control and batteries.
Plugs into a special connector on the control panel.
C Wall Adapter:Permits powering from a standard home (115v AC) outlet.
otater:
The field de-rotater attaches to the rear cell of the telescope
#1222 Field De-rotater: For use with the 16"
Fig. 46, page 49, to
RCX400 model.
Fig. 46,
Fig. 47: The Deep Sky Imager.
Astrometric Eyepiece: A high-precision 3-element achromatic eyepiece for a wide
range of astronomical measurements. Measure double star separations, position
angles, planetary diameters, lunar crater diameters and so forth. Includes variable
LED illumination control and batteries.
RCX Super Wedge: The equatorial wedge permits use of the RCX400 models in an
astronomical, or “equatorial,” mode. The superwedge fits onto the
Equatorial alignment allows you to take longer exposure photographs with your
RCX400. See APPENDIX A: EQUATORIAL (POLAR) ALIGNMENT, page 57 to 61, for fur-
ther information.
Deep Sky Imager: The Deep Sky Imager combines the power of an electronic astronomical imager with the simplicity of a web cam, allowing you to capture deep sky
images on your PC. See PHOTOGRAPHY WITH AUTOSTAR SUITE, pages 47 and 48, for
more information.
More accessories will soon be available for your
about these and other accessories available for your telescope, check out the Meade
General Catalog or contact your local Meade dealer. Also check out Meade’s latest
ads in Sky and Telescope and Astronomy magazine.
RCX400 model. To find out more
RCX tripod.
RCX400 TIPS
Star Charts
Even with the Autostar II's massive 180,000 object library, star charts and
planispheres are still useful for a variety of reasons. In particular, they are a
reat aid in planning a night of celestial vie
g
A wide variety of star charts are available in books, in magazines, on the internet and on CD Roms. Meade offers Autostar Suite and other star locator soft-
are. Contact your Meade dealer or Meade's Customer Service department
w
for more information.
elescope
Astronomyand Sky and
for up-to-the-minute maps of the heavens.
T
wing.
magazines pr
int star char
ts each month
50
MAINTENANCE
RCX400 telescopes are precision optical instruments designed to yield a lifetime of
rewarding applications. Given the care and respect due any precision instrument, your
RCX400 will rarely, if ever, require factory servicing. Maintenance guidelines include:
Avoid cleaning the telescope’s optics: A little dust on the front surface of the tele-
a.
scope’s correcting lens causes virtually no degradation of image quality and
should not be considered reason to clean the lens
b.When absolutely necessary, dust on the front lens should be removed with gen-
tle strokes of a camel hair brush or blown off with an ear syringe (available at any
pharmacy). DO NOT use a commercial photographic lens cleaner.
c.Organic materials (e.g., fingerprints) on the front lens may be removed with a
solution of 3 parts distilled water to 1 part isopropyl alcohol. You may also add 1
drop of biodegradable dishwashing soap per pint of solution. Use soft, white facial
tissues and make short, gentle strokes. Change tissues often.
Caution: Do not use scented or lotioned tissues or damage could result
to the optics.
d.Do not, for any reason, remove the correcting plate from its machined housing for
cleaning or other purposes. You will almost certainly not be able to replace the
corrector in its proper rotational orientation and serious degradation of optical
performance will result. Meade Instruments assumes no liability for damage
incurred to the telescope in this way.
e.If the
f.If your
g.Do not leave your
RCX400 is used outdoors on a humid night, water condensation on the tel-
escope surfaces will probably result. While such condensation does not normally
cause any damage to the telescope, it is recommended that the entire telescope
be wiped down with a dry cloth before the telescope is packed away. Do not, however, wipe any of the optical surfaces. Rather, simply allow the telescope to sit for
some time in the warm indoor air, so that the wet optical surfaces can dry unattended.
RCX400 is not to be used for an extended period, perhaps for one month
or more, it is advisable to remove the batteries from the telescope. Batteries left
in the telescope for prolonged periods may leak, causing damage to the telescope’s electronic circuitry.
RCX400 inside a sealed car on a warm summer day; excessive
ambient temperatures can damage the telescope’s internal lubrication and electronic circuitry
.
Collimation
The optical collimation (alignment) of any astronomical telescope used for serious purposes is important, but in the case of the RCX design, such collimation is absolutely
essential for good performance.Take special care to read and understand this section
well so that your telescope will give you the best optical performance.
As part of final optical testing, every Meade RCX400 telescope is precisely collimated
at the Meade factory before shipment. However, vibrations in shipping can cause the
optical system to become misaligned. Re-aligning the optics is, however, a straightforward process with the RCX400.
Test your Collimation
Before collimating your RCX400, you will need to test your collimation.
To test the collimation, center a bright star that is overhead, or use a “hot spot” of
reflected Sunlight from a chrome car bumper, with the supplied 24mm eyepiece. Allow
the telescope to adjust to the temperature of your observation site before proceeding;
temperature differences between the optics and the outside air can cause distortion in
the images. Autostar II offers two options in the Utilities menus that take temperature
readings: “OTA Temperature” (the temperature of the corrector plate) and “Ambient
(the temper
ature”
emper
T
When the star or hot spot is centered, de-focus the image.You will notice that the out
of focus star image looks like a ring of light surrounding a dark central spot; the dark
al spot is in f
centr
ature of the air around the f
act the shado
w of the secondar
.
k ar
or
y mirror
ms).
ou may notice multiple
Y
.
51
ings; these are called diffraction rings. Focus until the diffraction rings fills about 10%
r
of the eyepiece field-diameter. If the dark central spot is offset in (i.e., not concentric
with) the diffr
collimation.
w these steps for collimation of the optical system:
Follo
The only adjustments possible, or necessary, on the RCX400 models is performed
with the AutoStar handbox. No adjustment screws are necessary, as with traditional
telescopes
with a 2x barlow, is required for collimation. A good rule of thumb to follow is to select
the highest power eyepiece you will use with your telescope, and double it (a 2x barlow is ideal for doubling). See
aligned image.
a.Select the “Collimation” option in the Setup/Telescope menu. Once this option is
selected, you will be able to use Autostar’s Arrow keys to adjust the image of the
star you have selected.
b.While looking through the eyepiece, Use Autostar II's Arrow keys at the slowest
slew speed, begin to move the defocused center ring so that the rings become
more concentric. You will most likely need to press more than one Arrow key.
c.You will notice that the star image will move across the field of view of the eye-
piece. If while using the Arrow key, the defocused star image moves out of the
eyepiece field, press MODE to temporarily leave the collimation menu.
d.When you have left the “Collimation” menu, use the Arrow keys to bring the image
back to the center of the eyepiece field.
e.Press ENTER to select the “Collimation” option again.
f.Use the Arrow keys to continue to adjust the image until it become concentric. If
the image moves out of the eyepiece field, perform steps c through e as many
times as necessary.
g.Carefully examine the concentricity of the diffraction rings. Always double check
the image in the center of the field of the eyepiece. The star point should appear
as a small central dot (commonly referred to as an “Airy disc”) with a diffraction
ring surrounding it. You now have the best alignment of the optics possible with
this telescope.
action rings, your telescope’s optical system is misaligned and requires
. A high-powered eyepiece, such as a 9mm eyepiece, or a 9mm eyepiece
Fig. 48 below, to see images of an aligned and mis-
52
Set Default and Restore Default Options: The factory has collimated your telescope
ed the settings in the Restore Def
v
and sa
recall it if the telescope needs collimation. Or you may
ming precise collimation and recall it again when need
ault option after perf
Set Def
ed with the Restore Def
or
ault option.
ault option.
You may retain this setting and
overwrite this setting using the
123
Fig. 48: Defocused star images. Misaligned (1, 2), Aligned (3).
-
Inspecting the Optics
A Note about the “Flashlight Test:" If a flashlight or other high-intensity light source
is pointed down the main telescope tube, the view (depending upon the observer’s line
of sight and the angle of the light) may reveal what appear to be scratches, dark or
bright spots, or just generally uneven coatings, giving the appearance of poor quality
optics. These effects are only seen when a high intensity light is transmitted through
lenses or reflected off the mirrors, and can be seen on any high quality optical system,
including giant research telescopes
The optical quality of a telescope cannot be judged b
of optical quality can only be conducted through careful star testing.
.
y the “flashlight test;" the true test
Gauging the Movement of the Telescope
A common complaint of many first-time motorized telescope owners is that they cannot see the telescope “move” when the motor drive is engaged. If fact, when the batteries are installed, the power is on and the R.A. lock (
scope is moving. However, the movement is at the same speed as the hour hand of a
24-hour clock; as such, the movement is difficult to discern visually.
To check the movement of your telescope, look at an astronomical object through the
telescope’s eyepiece with the telescope aligned and with the motor drive on. If the
object remains stationary in the field of view, your telescope is operating properly. If
not, check to ensure that you have engaged the R.A. lock and that the power switch
on the control panel is on.
13, Fig. 1) engaged, the tele-
Meade Customer Service
If you have a question concerning your RCX400, contact the Meade Instruments
Customer Service Department at:
Telephone: (949) 451-1450
Customer Service hours are 7:00 AM to 6:00 PM, Pacific Time, Monday through
Friday. In the unlikely event that your RCX400 requires factory servicing or repairs,
write or call the Meade Customer Service Department first, before returning the telescope to the factory, giving full particulars as to the nature of the problem, as well as
your name, address, and daytime telephone number. The great majority of servicing
issues can be resolved by telephone, avoiding return of the telescope to the factory. If
factory service is required, you will be assigned a Return Goods Authorization (RGA)
number prior to return.
RCX400 TIPS
What is Smart Drive?
Smart Drive is a feature that allows you to train almost all of the periodic error from
the R.A. and Dec. motor drive worm gears. Periodic error is brought about by tiny
gear imperfections. These imperfections exist in all manufactured worm gears.
These imperfections tend to ever so slightly speed up or slow down the drive tracking speed during each rotation of the worm gear. This inconsistency in the tracking
rate can have a negative effect on astrophotography. Smart drive lets you train your
telescope system to compensate for these inconsistencies and, as a result, perform
more accurate tracking during astrophotography. Smart Drive remembers the training even after the telescope is turned off.
If you'd like to learn more about about Periodic Error Correction, see page 44.
or optional 115v AC cord
powered from auto cigarette lighter
UltraWide 24mm eyepiece, USB cable,
16-channel Sony GPS receiver,
extended sensitivity, magnetic declination
compensation
True-level and North electronic sensors
55
AUTOSTAR II SPECIFICATIONS
Advanced Autostar II System Specifications
Processors ........................................................10 processors arranged in a Distributed
The "Telescope: Mount"
option of the Setup menu is
set to "Alt/Az" as the default
mount by the factory.The
xample presented in this
e
section assumes that you are
performing an alignment procedure for the first time with
your telescope and therefore,
the "Telescope: Mount" option
does not need to be selected.
If the telescope is equatorially
mounted, y
ou must choose
the "Polar" option from the
Autostar II "Telescope Mount"
menu.
APPENDIX A: EQUATORIAL
(POLAR) ALIGNMENT
Equatorial Alignment
In equator
vertical axes of the telescope are lined up with the celestial coordinate system.
In order to equatorial align your telescope, it is essential to have an understanding of
how and where to locate celestial objects as they move across the sky. This section
provides a basic introduction to the terminology of equatorial-aligned astronomy, and
includes instructions for finding the celestial pole and for finding objects in the night
sky using Declination and Right Ascension.
Celestial Coordinates
A celestial coordinate system was created that maps an imaginary sphere surrounding the Earth upon which all stars appear to be placed. This mapping system is similar to the system of latitude and longitude on Earth surface maps.
In mapping the surface of the Earth, lines of longitude are drawn between the North
and South Poles and lines of latitude are drawn in an East-West direction, parallel to
the Earth’s equator. Similarly, imaginary lines have been drawn to form a latitude and
longitude grid for the celestial sphere.These lines are known as
Declination.
The celestial map also contains two poles and an equator just like a map of the Earth.
The poles of this coordinate system are defined as those two points where the Earth’s
North and South poles (
celestial sphere. Thus, the North Celestial Pole (
where an extension of the North Pole intersects the celestial sphere. The North Star,
Polaris, is located very near the North Celestial Pole (
tor (
So just as an object's position on the Earth’s surface can be located by its latitude and
longitude, celestial objects may also be located using Right Ascension and
Declination.
(+34°) and longitude (118°). Similarly, you could locate the Ring Nebula (M57) by its
Right Ascension (18hr) and its Declination (+33°).
ial (or "polar") Alignment, the telescope is oriented so that the horizontal and
Right Ascension and
i.e., the Earth's axis), if extended to infinity, would cross the
1, Fig. 49) is that point in the sky
1, Fig. 49). The celestial equa-
2, Fig. 49) is a projection of the Earth’s equator onto the celestial sphere.
For example: You could locate Los Angeles, California, by its latitude
Fig. 49: Celestial Sphere.
JRight Ascension (R.A.): This celestial version of longitude is measured in units
of hours (hr), minutes (min), and seconds (sec) on a 24-hour "clock" (similar to
how Earth's time zones are determined by longitude lines). The "zero" line was
ily chosen to pass through the constellation P
ar
arbitr
R.A. coordinates range from 0hr 0min 0sec to 23hr 59min
Greenwich mer
There are 24 pr
59sec.
the celestial equator
line (0hr 0min 0sec) carr
idian.
imar
Objects located fur
.
y higher R.A. coordinates.
y lines of R.A., located at 15-deg
ther and fur
egasus, a sort of cosmic
als along
ree inter
v
ther East of the zero R.A. grid
JDeclination (Dec.): This celestial version of latitude is measured in degrees, arc-
minutes, and arc-seconds (
e.g., 15° 27' 33"). Dec. locations North of the celestial
equator are indicated with a plus (+) sign (e.g., the Dec. of the North celestial pole
). Dec. locations South of the celestial equator are indicated with a minus
°
is +90
(–) sign (
e.g., the Dec. of the South celestial pole is –90°). Any point on the celestial equator (such as the the constellations of Orion, Virgo, and Aquarius) is said
to have a Declination of zero, shown as 0° 0' 0."
Setting Circles
Setting circles included with the RCX400 models permit the location of faint celestial
objects not easily found by direct visual observation.The R.A. circle (
ed on the top surface of the telescope’s drive base. The Declination circle (
located at the top of the fork tine. With the telescope pointed at the North Celestial
Pole, the Dec. circle should read 90° (understood to mean +90°). Objects located
below the 0-0 line of the Dec. circle carry minus Declination coordinates. Each division
of the Dec. circle represents a 1° increment. The R.A. circle runs from 0
including) 24
hr
, and reads in increments of 5
min
.
Fig. 51) is locat-
Fig. 50) is
hr
to (but not
57
Using setting circles requires a de
first time, try hopping from one bright star (the calibration star) to another bright star
wn coordinates. Practice moving the telescope from one easy-to-find object to
of kno
another. In this way, the precision required for accurate object location becomes evident.
Note You may also enter an object's R.A. and Dec. coordinates using the
"User: Objects" option of Autostar II's Object menu. Autostar II then automatically slews the telescope to the entered coordinates.
veloped technique. When using the circles for the
50:
Fig.
Declination Setting Circle
Fig. 51: Section of Right Ascension
Setting Circle.
Note that the R.A. circle is double-indexed (i.e., there are two series of numbers run-
ning in opposite directions around the circumf
series of numbers (increasing counterclockwise) applies to observers located in the
Earth’s Northern Hemisphere; the lower series of numbers (increasing clockwise)
applies to observers located in the Earth’s Southern Hemisphere.
To use the setting circles to locate an object not easily found by direct visual
observation:
.
With the telescope aligned to the Celestial P
(R.A. and Dec.) of the object in a star atlas. Then loosen the R.A. lock and move the
telescope to read the correct R.A. of the desired object; lock the R.A. lock onto the
coordinate. Next, move the telescope in Declination to read the correct Declination of
the object. If the procedure has been followed carefully, and if the telescope was wellaligned with the pole, the desired object should now be in the telescopic field of a lowpower eyepiece.
If you do not immediately see the object you are seeking, try searching the adjacent
sky area. Keep in mind that, with the 24mm eyepiece, the field of view of the
is about 0.75°. Because of its much wider field, the viewfinder may be of significant
assistance in locating and centering objects, after the setting circles have been used
to locate the approximate position of the object.
Pinpoint application of the setting circles requires that the telescope be precisely
aligned with the pole. See
PRECISE POLAR ALIGNMENTS, page 60.
erence of the R.A. circle). The upper
ole, first look up the celestial coordinates
RCX400
Equatorial Wedge
An optional equatorial RCX superwedge is required for equatorial (polar) alignment.
See Fig. 54.
The equatorial wedge permits use in an astronomical, or “equatorial,” mode. The
wedge fits onto the field tripod. Equatorial alignment allows you to take longer exposure photographs with your
See the instruction sheet supplied with the wedge for installation and setup information.
Note: For almost all astronomical observing requirements, approximate settings of the telescope’
undue attention to precise polar alignment of the telescope to interf
your basic enjoyment of the instrument.
Note: The Meade equator
with your Meade tripod. The wedge should never be used without the tripod
(e.g., by placing the wedge alone on a table top and then mounting the telescope on the wedge—the wedge may become seriously unbalanced, to the
point where the telescope ma
Included features:
RCX400.
s latitude and polar axis are acceptable. Do not allow
ere with
edge is designed solely for use in conjunction
ial w
y actually tip o
ver.
58
y means of only one man
JAttachment of the w
JQuic
JBubble level for rapid tripod/wedge leveling.
JEtched latitude scale f
k azimuth adjustment by loosening the manual knob.
edge to the tr
ast adjustment of the latitude angle
or f
ipod b
.
ual knob
.
P
olaris
Little Dipper
B
ig Dipper
Cassiopeia
Fig. 52: Locating Polaris.
Tip:
You can check if the declination is set at true 90° in step
2c. Look through the eyepiece
and rapidly slew the optical
tube on the R.A. axis.If all the
stars rotate around the center
of the field of view, the
Declination is set at 90°. If the
stars arc out of the field of
view, slew the optical tube on
the Declination axis until you
achieve the centering effect.
C
A
B
Fig. 53: Align tick marks to set the
fork arms to 00 H.A. position.
Lining Up with the Celestial Pole
Objects in the sky appear to revolve around the celestial pole. (Actually, celestial
objects are essentially
During any 24 hour period, stars make one complete revolution about the pole, making concentr
with the North Celestial Pole (or for observers located in Earth’s Southern
Hemisphere, with the South Celestial Pole), astronomical objects may be followed, or
tracked, simply by moving the telescope about one axis, the polar axis. This tracking
may be accomplished automatically with the
If the telescope is reasonab
scope’s Declination slow motion control is necessary. Virtually all of the required telescope tracking will be in Right Ascension. (If the telescope were perfectly aligned with
the pole, no Declination tracking of celestial objects would be required.) For the purposes of casual telescopic observations, lining up the telescope’s polar axis to within
a degree or two of the pole is more than sufficient: with this level of pointing accuracy, the telescope’s motor drive will track accurately and keep objects in the telescopic field of view for perhaps 20 to 30 minutes.
Begin polar aligning the telescope by locating Polaris. Finding Polaris is simple. Most
people recognize the “Big Dipper.” The Big Dipper has two stars that point the way to
Polaris (
rough polar alignment.
To line up with Polaris, follow the procedure described below. Refer to the instruction
sheet included with your equatorial wedge for information about attaching the wedge
to the telescope and also about using the azimuth and latitude controls.
1.Select "Setup: Telescope" from the Autostar II menus. Press ENTER. Scroll to
"Telescope: Mount" and press ENTER. Scroll to "Scope Mounting: Polar" and
press ENTER. The telescope mount is now set to the polar mode.
2.Press MODE until "Select Item: Setup" displays. Press ENTER. "Setup: Align" displays. Press ENTER. "Align: Easy" displays. Scroll to "Align: One-Star" and press
ENTER. Autostar II now prompts you to set the telescope in the polar home position.
a.Using the bubble level of the wedge, adjust the tripod legs so that the
b.Set the wedge to your observing latitude.
c.Using the Up and Down Arrow keys, rotate the telescope tube in Declination
d.Loosen the R.A. lock, and rotate the fork arms to the 00 position H. A. : Move
e.Press ENTER. The telescope slews to Polaris.
f.Use the azimuth and latitude controls on the wedge to center Polaris in the
field of view. Do not use the Autostar II handbox during this process. When
Polaris is centered, press ENTER. The telescope is now polar aligned. See
AUTOSTAR II PRECISE POLAR ALIGNMENT, page 60, for more information.
At this point, your polar alignment is good enough for casual observations. There are
times, however, when you will need to have precise polar alignment, such as when
making fine astrophotographs.
Once the latitude angle of the wedge has been fixed and locked-in according to the
above procedure, it is not necessary to repeat this operation each time the telescope
is used, unless you move a considerable distance North or South from your original
obser
tion is equiv
ipod and, as long as the latitude angle setting is not altered and the field tr
tr
eled, it will retain the correct latitude setting when replaced on the tr
ic circles with the pole at the center. By lining up the telescope’s polar axis
Fig. 52). Once Polaris is found, it is a straightforward procedure to obtain a
bubble is level.
so that the telescope’s Declination reads 90°. See
the forks arms so that center tick mark on fork arm base (A, Fig. 53) aligns
with the tick mark on the base (B, Fig. 53).
ving position.
alent to 1
“fixed.” Their apparent motion is caused by the Earth’s rotation).
RCX400 electric motor drive.
ly well aligned with the pole, very little use of the tele-
SETTING CIRCLES, page 57.
ximately 70 miles mo
(Appro
in latitude change
°
The w
.)
ement in Nor
v
edge may be detached from the field
th-South obser
ving posi
ipod is le
ipod.
-
-
v
The first time you polar align the telescope, check the calibration of the Declination
setting circle (
is in the telescope field.
olar
P
Fig. 50). After performing the polar alignment procedure, center the star
Remo
e the kn
v
urled central hub of the Declination set-
59
Fig. 54: RCX400 mounted on an
equatorial wedge.
ting circle and slightly
unit until it reads 89.2°, the Declination of Polaris.Then tighten down the two bolts and
replace the kn
Should you wish to use the manual setting circles, the R.A. setting circle (
be calibrated manually on the Right Ascension of a star every time the telescope is set
up. (The R.A. setting circle has two sets of numbers, the inner set is for Southern
hemisphere use, while the other is for Northern hemisphere use.) Locate a star with
which y
star centered in the telescope's eyepiece, move the R.A. setting circle, using one of
knobs (
of the telescope (B, Fig. 53).
urled knob.
ou're familiar. Look up the R.A. for the star in a star chart or other aid. With the
C, Fig.53), so that the R.A.
loosen the two bolts located under the knob. Now turn the circle
Fig. 51) must
of the star lines up with the tick mark on the base
Precise Polar Alignment
It should be emphasized that while doing casual observing, precise alignment of the
telescope’s polar axis to the celestial pole is not necessary. Don’t allow a time-consuming effort at lining up with the pole to interfere with your basic enjoyment of the telescope. For long-exposure photography, however, the ground rules are quite different,
and precise polar alignment is not only advisable, but almost essential.
Even though the
tem, the fewer tracking corrections required during the course of a long-exposure photograph, the better. (“Long-exposure” means any photograph of a celestial object that
last for 10 minutes or longer). In particular, the number of Declination corrections
required is a direct function of the precision of polar alignment.
Precise polar alignment requires the use of a crosshair eyepiece. The Meade
Illuminated Reticle Eyepiece (see
suited in this application, but it is also preferable to increase the effective magnification through the use of a 2X or 3X Barlow lens as well. Follow this procedure (particularly if the pole star is not visible), sometimes better known as the “Drift” method:
1.Obtain a rough polar alignment as described earlier. Place the illuminated reticle
eyepiece (or eyepiece/Barlow combination) into the eyepiece holder of the telescope.
2.Point the telescope, with the motor drive running, at a moderately bright star near
where the meridian (the North-South line passing through your local zenith) and
the celestial equator intersect. For best results, the star should be located within
±30 minutes in R.A. of the meridian and within ±5° of the celestial equator (see
CELESTIAL COORDINATES, page 57). Pointing the telescope at a star that is
straight up, with the Declination set to 0°, will point the telescope in the right direction.
3.Note the extent of the star’s drift in Declination (disregard drift in Right Ascension):
a.If the star drifts South (or down), the telescope’s polar axis is pointing too far
East.
b.If the star drifts North (or up), the telescope’s polar axis is pointing too far
West.
4.Move the wedge in azimuth (horizontally) to effect the appropriate change in polar
alignment. Reposition the telescope’s East-West polar axis orientation until there
is no further North-South drift by the star. Track the star for a period of time to be
certain that its Declination drift has ceased.
5.Next, point the telescope at another moderately bright star near the Eastern horizon, but still near the celestial equator. For best results, the star should be about
20° or 30° above the Eastern horizon and within ± 5° of the celestial equator.
6.Again note the extent of the star’s drift in Declination:
a.If the star drifts South, (or down) the telescope’s polar axis is pointing too low.
b.If the star drifts North, (or up) the telescope’s polar axis is pointing too high.
7.Use the altitude adjust control on the wedge to make appropriate changes in altitude
, based on your observations above. Again, track the star for a period of time
to be cer
e procedure results in v
The abo
or tr
f
v
king corrections during astrophotography.
ac
RCX400 telescopes offers a very precise and sophisticated drive sys-
OPTIONAL ACCESSORIES, pages 48 - 50) is well-
tain that Declination dr
ift has ceased.
y accur
er
ate polar alignment, and minimizes the need
60
Important Note:
In order to select any of
Autostar II's three polar
alignment options, you must
first select "Polar" in the
"Mount" option of the
"Setup: Telescope" menu.
Autostar II Polar Alignment
utostar II provides three different (manual) methods for polar alignment: Easy, One-
A
Star and Two-Star.
Easy Polar Alignment
Two alignment stars are chosen by Autostar II based on the date, time, and location.
First, choose "Polar" from the "Setup: Telescope: Mount" menu.The rest of the procedure is identical to the (Alt/Az)
EASY (TWO-STAR) ALIGN, page 42.
One-Star Polar Alignment
Polar One-Star Alignment requires some knowledge of the night sky. Autostar II provides a library of bright stars and one star from this library is chosen by the observer
for alignment. Polaris is chosen by Autostar II. First, choose "Polar" from the "Setup:
Telescope: Mount" menu. The rest of the procedure is almost identical to the (Alt/Az)
ONE STAR ALT/AZ ALIGNMENT, page 43, except that Autostar II prompts you to point
the telescope at Polaris and center it in the telescope eyepiece.
Two-Star Polar Alignment
Polar Two-Star Alignment requires some knowledge of the night sky. Autostar II provides a libr
er for alignment. First, choose "Polar" from the "Setup: Telescope: Mount" menu. The
rest of the procedure is almost identical to the (Alt/Az)
page 42.
ary of bright stars and two stars from this library are chosen by the observ-
TWO STAR ALT/AZ ALIGNMENT,
RCX400 TIPS
Surf the Web
One of the most exciting resources for astronomy is the internet. The internet is full
of websites with new images, discoveries, and the latest astronomical information.
For example: When comet Hale-Bopp made its approach to our Sun in 1998,
astronomers around the w
On the internet, you can find websites for almost any topic relating to astronomy. Try
the following key word searches: NASA, Hubble, HST, astronomy, Messier, satellite,
nebula, black hole, variable stars, etc.
Check Meade’s website for the latest product and technical information. You can
download the latest software revisions, links to other astronomical sites, coordinates
of celestial objects and the latest satellite tr
x. See page 35 for more information. You’ll find our website at:
handbo
www.meade.com/
Here are some other sites you might find interesting:
• Sky & Telescope:
http://www.SkyandTelescope.com
• Astronomy:
http://www.astronomy.com
The Starfield:
•
http://users.nac.net/gburke/
• Astronomy Picture of the Day:
http://antwr
ens Above (satellite observing information):
v
• Hea
http://www.heavens-above.com
• Photographic Atlas of the Moon:
http://www.lpi.ursa.edu/research/lunar_orbiter
• Hubble Space Telescope Public Pictures
http://oposite
.gsfc.nasa.goc/apod
p
.stsci.edu/pubinf
orld posted new photos daily.
king inf
ac
o/pictures
.html
ormation for your Autostar II
61
APPENDIX B: LATITUDE CHART
Latitude Chart for Major Cities of the World
To aid in the polar alignment procedure (see page 57), latitudes of major cities around the world are listed below. To determine the latitude of
an observing site not listed on the chart, locate the city closest to your site. Then follow the procedure below:
Northern hemisphere observers (N): If the site is over 70 miles (110 km) North of the listed city, add one degree for every 70 miles. If the
site is over 70 miles South of the listed city, subtract one degree per 70 miles.
Southern Hemisphere observers (S): If the site is over 70 miles (110 km) North of the listed city, subtract one degree for every 70 miles. If
the site is over 70 miles South of the listed city, add one degree per 70 miles.
NORTH AMERICA
CityState/Prov./Country Latitude
AlbuquerqueNew Mexico35° N
AnchorageAlaska61° N
AtlantaGeorgia34° N
BostonMassachusetts42° N
CalgaryAlberta51° N
Chicago
ClevelandOhio41° N
Dallas
DenverColorado40° N
DetroitMichigan42° N
HonoluluHawaii21° N
JacksonMississippi32°N
Kansas CityMissouri39° N
KenoshaWisconsin45° N
Las VegasNevada36° N
Little RockArkansas35° N
Los AngelesCalifornia34° N
Mexico CityMexico19° N
MiamiFlorida26° N
MinneapolisMinnesota45° N
NashvilleTennessee36° N
New OrleansLouisiana30° N
New YorkNew York41° N
Oklahoma CityOklahoma35° N
OttawaOntario45° N
PhiladelphiaPennsylvania40° N
PhoenixArizona33° N
PortlandOregon46° N
Salt Lake CityUtah41° N
San AntonioTexas29° N
San DiegoCalifornia33° N
San FranciscoCalifornia38° N
Seattle
WashingtonDistrict of Columbia39° N
OPE
EUR
Illinois42° N
Texas33° N
°
ashington
W
47
N
CityCountryLatitude
AmsterdamNetherlands52° N
Athens
BernSwitzerland47° N
CopenhagenDenmark56° N
DublinIreland53° N
FrankfurtGermany50° N
GlasgowScotland56° N
Helsinki
Lisbon
London
MadridSpain40° N
OsloNorway60° N
ParisFrance49° N
RomeItaly42° N
StockholmSweden59° N
Vienna
Warsaw
Greece
Finland
tugal
or
P
England
ia
ustr
A
oland
P
°
38
°
60
°
39
°
51
°N
48
52° N
N
N
N
N
SOUTH AMERICA
CityCountryLatitude
BogotáColombia4° N
São PauloBrazil23° S
Buenos AiresArgentina35° S
videoUruguay35° S
Monte
SantiagoChile34° S
CaracasVenezuela10° N
ASIA
CityCountryLatitude
BeijingChina40° N
Hong KongChina23° N
SeoulSouth Korea37° N
TaipeiTaiwan25° N
TokyoJapan36° N
SapporoJapan43° N
BombayIndia19° N
CalcuttaIndia22° N
HanoiVietnam21°N
JeddaSaudi Arabia21° N
AFRICA
CityCountryLatitude
CairoEgypt30° N
Cape TownSouth Africa34° S
RabatMorocco34° N
TunisTunisia37° N
WindhoekNamibia23° S
AUSTRALIA AND OCEANIA
CityState/CountryLatitude
AdelaideSouth Australia35° S
BrisbaneQueensland27° S
CanberraNew South Wales35° S
Alice SpringsNorthern Territory24° S
HobartTasmania43° S
n Australia32° S
ester
th
er
P
y
Sydne
MelbourneVictoria38° S
AucklandNew Zealand37° S
W
New South Wales34° S
62
APPENDIX C: CREATE
YOUR OWN GUIDED TOUR
Creating your own Guided Tour can be an extremely useful tool. You can preprogram a
ipt of objects you wish to view and study on any given night. You can also create a
scr
viewing script for students or for a friend.
More commands will be added from time-to-time to the list belo
Meade's website (www.meade.com) for future additions.
When a Guided Tour is selected, Autostar II slews your telescope to a predetermined
list of objects and displa
stellation location, R.A. and Dec. coordinates, and so forth. Autostar II contains a few
Guided Tours which are programmed at the factory. But it is also possible for an observer to create a custom Guided Tour.
A tour is basically an ASCII text file that contains a list of directions and descriptions.
Each line of a tour is either a comment line, a command line, or a description.
What you will need:
JA PC with text editor or word processing software installed (the tour must be
saved as a "text only" or as a "MS-DOS text" file).
JThe optional Meade RCX400 Interface Cable to download tour information to the
Autostar II handbox.
Tour Modes
The objects chosen for a tour list are selected from Autostar II's database or by entering the object's R.A. and Dec. coordinates. The tour is presented in one of two modes:
Automatic Mode: The title of an object appears on first line and descriptive text scrolls
on line 2.
Interactive Mode: Tour name appears on the first line of the Autostar II display and the
name of the object displays on line 2. To display descriptive text in this mode, the user
must press ENTER.
Comment Line
Information in the Tour program that is not displayed, such as authorship, revision history, copyrights, etc. All comments begin with a "/" character in column 1 of the line.
For example:
ys information about each object, such as type of object, con-
This line contains prog
title string, a description string, and a keyword.
R.A.: Enter the Right Ascension of an object in the f
Eg., 18:51:05
Dec.: Enter the Declination of an object in the f
06d16m00s
Title String: Text within a title string is displayed as the title of the object. A title string
can contain up to 16 char
xample:"M64" or "My F
e
In
Interactive Mode, the title string appears on line 2 until it is selected with the ENTER
.
y
e
k
In
Automatic Mode, or after Interactive Mode selection, the title string appears on line
1 while the description scrolls across line 2.
eywords:Action to be performed during a tour. Autostar II recognizes the following
K
keywords:
r
acters and m
vorite Star."
a
, including:
wing f
ollo
ust be surrounded b
R.A. and Dec. coordinates, a
mat: HH:MM:SS.
or
wing f
ollo
or
mat:
DDdMMmSSs
y quotation mar
.
Eg., –
ks
.
or
F
63
TITLETEXTUSERNGC
ICSAOMESSIERCALDWELL
PLANETMOONSATELLITEASTEROID
COMETLUNAR ECLIPSE METEOR SHOWER DEEP SKY
CONSTELLA
PICK ONE/PICK END AUTO SLEW ON/OFF#END
Description String: Description of an object. Must be surrounded by quotation marks.
If the descr
a hard return. Begin the next description line with a quotation mark.
If quotation marks are to be displayed in the on-screen description, use two quote
marks at the beginning and end of the desired phrase.
Nebula is considered ""awesome"" by many who view it."
Writing a Tour
Using the list of commands listed above, a custom tour can be created. Placing the
word AUTO SELECT before any of the command lines activates Automatic Mode and,
when selected, Autostar II automatically searches and finds the designated object.
The following is a list of command lines, complete with keywords and necessary
strings:
TITLE
Title must be the first keyword in your tour after any comment lines and must be 15
characters or less. Autostar II displays this title when "Guided Tour" is selected from
the menus.
For example: TITLE "A Star's Life"
TEXT "title string" "description string"
This command allows you to display a text title and description.
TIONSTARLANDMARKDEFINE
iption is longer than one line, each line must end with a quotation mark and
For example: "The Orion
USER ra dec "title string" "description string"
This command line allows you to access a specific object with your own description.
Enter USER, then the R.A. and Dec. of a desired object, and its title and description.
Use the format described in the Command Line section.
The following commands specify objects that are already in the Autostar II database.
If these commands follow the command AUTO SELECT, the object's title displays on
line 1 and its description scrolls across line 2.
Do not add a description string after the following command lines; these commands
access objects with existing description in the Autostar II database.
NGC xxxx
Enter NGC followed by the desired New General Catalog number and Autostar II provides the user with a description of the object from its database.
4256
IC xxxx
Enter IC followed by the desired Index Catalog number and Autostar II provides the
user with a description of the object from its database.
SAO xxxxxx
Enter SAO followed by the desired SAO number and Autostar II provides the user with
a description of the object from its database.
Messier xxx
Enter MESSIER followed by the desired Messier number and Autostar II provides the
user with a description of the object from its database.
For example: SAO 30200
For example: IC 1217
For example: M 101
For example: NGC
64
CALDWELL xxx
Enter CALD
with a descr
WELL followed by the Caldwell number and Autostar II provides the user
iption of the object from its database
xample:
or e
.
F
CALD
WELL 17
PLANET "name"
Enter PLANET and then the name of the desired planet in quotes. Autostar II provides
the user with a descr
PLANET "Pluto"
MOON
This command accesses information about the Moon from the Autostar II database.
SATELLITE "name"
Enter SATELLITE and then the name of the desired satellite in quotes. Autostar II displays information about the satellite from its database.
Space Stn"
OID "name"
ASTER
Enter ASTEROID and then the name of the desired asteroid in quotes. Autostar II displays information about the asteroid from its database.
"Ceres"
COMET "name"
Enter COMET and then the name of the desired comet in quotes. Autostar II displays
information about the comet from its database.
LUNAR ECLIPSE
If LUNAR ECLIPSE is part of the tour, Autostar II checks its database every time the
tour is activated to see if a lunar eclipse is visible that evening. If no eclipse is visible,
this option is skipped and the tour proceeds on to the next object.
METEOR SHOWER
If METEOR SHOWER is part of the tour, Autostar II checks its database every time
the tour is activated to see if a meteor shower is visible that evening. If no meteor
shower is visible, this option is skipped and the tour proceeds on to the next object.
iption of the selected planet from its database.
For example: SATELLITE: "Intl
For example: ASTEROID:
For example: COMET: "Halley"
or example:
F
DEEP SKY "name"
Enter DEEP SKY followed by the name of the desired object in quotes.
DEEP SKY "Small Magellanic Cloud"
CONSTELLATION "name"
Enter CONSTELLATION followed by the name of the desired constellation in quotes.
For example: CONSTELLATION "Leo Major"
STAR "name"
Enter STAR followed by the name of the desired star in quotes. For example: STAR
"Vega"
LANDMARK az alt "title" "description"
Enter the azimuth (az) for the desired object in the following format: xxxdxxmxxs.
example:
format: xxdxxmxxs. Then enter the title string and description string in quotes.
example:
LANDMARK 123d27m00s 57d20m20s "Landmark 1" "North corner of apartment
building"
PICK ONE / PICK END
These tw
from dur
first object from the list that is above the horizon and ignores the rest.
This statement is useful f
each object type you wish to use to illustrate in your tour, pick 10 to 12 examples
spaced across the range of right ascension. Bracket them by the PICK ONE / PICK
END statements
UT
A
"The
"galaxy."
123d27m00s. Then enter the altitude of the desired object in the following
o statements are used to surround a list of items that A
ing a tour
O SELECT TEXT "Globular Cluster" "Globular clusters are huge balls of stars."
y contain 50,000 to 100,000 stars and are located on the fringes of our"
. Autostar II begins at the top of the PICK ONE list and displays the
eloping tours that can be presented y
v
or de
or the user
One current e
.
xample displa
ys f
utostar II can choose
.
or e
F
For example:
For
For
ear-round. For
xample:
65
PICK ONE
AUTO SELECT MESSIER 13
AUTO SELECT MESSIER 15
AUTO SELECT MESSIER 92
UTO SELECT MESSIER 4
A
AUTO SELECT MESSIER 68
UTO SELECT NGC 1234
A
AUTO SELECT TEXT "None Available" "I'm sorry. There are no bright globular"
"clusters visib
PICK END
AUTO SLEW ON / AUTO SLEW OFF
With AUTO SLEW ON enabled in the tour, Autostar II automatically slews the telescope to objects first before displaying the text description. This feature is useful when
designing tours in which observing certain objects is required.
astronomy professor may require his students to observe six objects, four of which
Autostar II automatically slews to in a tour. The students would have to manually slew
to the last two objects. He would then place AUTO SLEW ON before his first required
object and AUTO SLEW OFF after the fourth object.
#END
To end a tour, type the command #END on a separate line at the very end of the tour.
Downloading Tours
Once a tour is written and stored as an ASCII file (saved either as a "text only" or "MS
DOS text" file), load it into Autostar II using the Autostar II Update Utility on your PC.
As tours are downloaded into the handbox, Autostar II examines the programming. If
it doesn't understand the terminology used within a tour, it flags questionable areas
and displays them in a pop-up window on your computer screen. Make the necessary
corrections and try to download again. See the instruction sheet with your
Interface Cable for more information about downloading data to and interfacing with
Autostar II.
le at this time."
For example:An
RCX400
66
Press > until it
i
s centered
Press < until it
is centered
T
rain Drive
Az. Train
Train Drive
Alt. Train
Drive Setup
For this op. . .
Center reference
object
ENTER
ENTER
ENTER
ENTER
S
cope slews left.
Bring target back
to center using
t
he Right Arrow key.
12
1
3
1
4
15
16
17
Scope slews right.
Bring target back
t
o center using
t
he Left Arrow key.
Menu returns to
Az. training.
Altitude
(vertical)
training.
Reminder to
use terrestrial
target.
Train Drive
Az. Train
Select Item
Object
Press until it
is centered
Press until it
is centered
ENTER
ENTER
MODE
18
19
20
21
Center target
using Arrow
keys.
Scope slews down.
Bring target back
to center using
the Up Arrow key.
Scope slews up.
Bring target back
to center using
the Down Arrow key.
Multiple presses.
ENTER
Select Item
Object
Select Item
Setup
Setup
Align
Setup
Telescope
3
4
6
ENTER
Press the scroll
up key once.
Access the Setup
m
enu.
M
ultiple presses.
Access the
Telescope menu.
5
ENTER
1
Telescope
Telescope Model
Telescope
Train Drive
Train Drive
Az. Train
Drive Setup
For this op. . .
Center reference
object.
ENTER
ENTER
ENTER
Multiple presses.
Choose the Train
Drive option.
Azimuth
(horizontal)
training.
7
8
9
10
11
Reminder to
use terrestrial
target.
Center target
using Arrow
keys.
ENTER
Verify that AUTOSTAR
INITIALIZATION is
complete.
P
ress MODE until
Select Item is displayed.
1
2
>
>
APPENDIX D: TRAINING THE DRIVE
Train the telescope motors using Autostar II. Perform this procedure if you are experiencing any pointing accuracy
prob
Figure 55: Training the Drive Procedure.
lems.
Fig.55depicts the complete Dr
ive Training procedure.
Note: Use a terrestrial object, such as a telephone pole or lamp post, to train the drive. Complete this exer-
cise once every 3 to 6 months to maintain the highest level of telescope pointing accuracy.
RCX400 TIPS
Further Study....
This manual gives only the briefest introduction to astronomy. If you are interested in pursuing further studies in
astronomy, a few topics are suggested below that are
worth reading up on. Try looking up some of these in the
optional Autostar II glossary.
Also included below is a small sampling of books, magazines, and organizations that you might find helpful.
Topics
1.How is a star born? How does a solar system form?
2.How is the distance to a star measured? What is a
light year? What is red shift and blue shift?
3.How are the craters on our Moon formed? Is there
water under the surface of the Moon?
What is a black hole? A neutron star? A quark star?
4.
A gamma burster? An Einstein lens?
5.What are stars made of? Why are stars different colors? How is the elemental composition of a star
determined? What is an Lyman Alpha forest?
6.What is the difference between a Type 1 and a Type
II supernova?
7.What is the importance of studying the composition
of comets? Where do comets come from?
8.How old is our Sun? Will our Sun evolve into a planetary nebula or go supernova?
9.What is the Inflationary Big Bang? What is dark matter? What are MACHO's?
10. How are extrasolar planets discovered? What is an
accretion (or protoplanetary) disk?
11. What are the differences between elliptical, spiral,
and irregular galaxies?
12. Have we discovered proof that water exists anywhere else in our solar system?
Books
The Guide to Amateur Astronom
1.
and Philip Teece
The Sky: A User’s Guide by David Levy
2.
urn Left at Orion by Guy Consolmagno & Dan Davis
3.
T
4.
Astrophotog
vington
Co
raphy for the Amateur by Michael
Magazines
1.Sky & Telescope
Box 9111, Belmont, MA 02178
2.Astronomy
Box 1612, Waukesha, WI 53187
ganizations:
Or
1.Astronomical League
Ex
ecutiv
e Secretar
y
5675 Real del Norte, Las Cruces, NM 88012
2.The Astronomical Society of the Pacific
390 Ashton A
The Planetar
3.
ve., San Francisco, CA 94112
y Society
65 North Catalina Ave, Pasadena., CA 91106
And watch Jack Horkheimer,
Star Gazer, on your local
PBS station.
by Jack Newton
y
67
APPENDIX E: THE MOON MENU
The Moon option of the Object menu allows you to observe the moon in a way never
possible before. You will be able locate many specific features of the lunar surface,
including hundreds of craters, mare, valleys, and mountains. One special feature
allows you to view all six Apollo landing sites. While you won't be able to see details
such as any of the lunar landers or lunar excursion modules left behind by the astronauts (the best earth-based telescopes can only resolve features of about a half-mile
across), you'll be able pinpoint the landing sites and study the terrain surrounding
these sites
When Autostar II synchs to a lunar feature, the telescope switches to Selenographic
coordinates,
o observe the Apollo 15 landing site using the Moon option:
T
1. Initialize and align the telescope system as previously described.
2. Press "5" on the Autostar II keypad. "Solar System: Mercury" displays.
3. Press a Scroll key until "Solar System: Moon" displays. Press ENTER.
4.
5. With "Moon: Overview" on Autostar II's display, use the Scroll keys to browse
6. Select a distinct lunar crater with which you are familiar, such as Copernicus or
7. Then press GO TO to slew to that feature. Center the feature in the eyepiece
8. Press MODE twice to return to the features list. Press a Scroll key until "Moon:
9. Press ENTER. "Landing Sites: Apollo 11" displays.
10. Press a Scroll key until "Landing Sites: Apollo 15" displays.
11. Press GO TO. The telescope slews to the Apollo 15 site.
12. Press MODE to return to the previous menu option. Continue to press MODE to
Use this method to find other lunar features and points of interest. When you have
selected a feature, press the "?" key or use the Scroll keys to display detailed information about the feature. Press MODE to return to the menu options.
.
i.e., lunar latitude and longitude.
"Moon: Overview" displays. Press GO TO. The telescope slews to the Moon.
through the menus options. Five categories of features are available: Landing
Sites, Craters, Mountains, Mare and Lakes, and Valleys and Rills.
Kepler, from the Craters option and press ENTER.
and hold down ENTER for more than two seconds to ENTER TO SYNC. The
telescope is now synced to Selenographic coordinates.
Landing Sites" displays.
exit this menu.
68
Kepler
Copernicus
Tycho
Figure 56: Some easily recognized lunar craters.
APPENDIX F:
Smart Mount
oduction
Intr
Smart Mount improves the pointing accuracy of your RCX400 telescope's "Go to" sys-
Despite careful efforts to calibrate and align telescopes, they may fail to
tem.
precisely center objects. Smart Mount allows your telescope to learn about, and then
correct for, any systematic pointing errors, regardless of the cause.
Because training your mount takes some time, we recommend that it be primarily
used on permanently mounted instruments or when imaging requires very accurate
pointing.
it so long as you carefully park the telescope at the end of each session and do not
modify the mounting.
For portable instruments, we recommend training Smart Mount each time you set up
your telescope to insure best results.
Once Smart Mount training has been performed, the scope will benefit from
Want to learn more
about Alignment?
See page 22.
Want to learn more
about
training your
? See page 67.
drive
We recommend that you use an
illuminated reticle allows you to precisely center celestial objects in a telescope’s
eyepiece. The more precisely you center objects during Smart Mount training, the
more pointing precision your telescope will be able to achieve. If you do not have an
illuminated reticle, see
Operation
The Smart Mount feature is located in the Autostar II Setup menu.
In order to use Smart Mount, create a model that allows Smart Mount to improve your
telescope's accuracy. This is normally done by training Smart Mount. Once training
has been completed, you will save your model. Autostar II allows you to save
several models under different names. This allows you to, for example, save one
model for a heavy imaging camera configuration on a permanently aligned scope, and
another when you have a lighter load on the mount.
Training
In order to obtain solid, repeatable results, perform the following procedures before
you create a model:
Setup and align your telescope.
•
• Perform both RA/Az and Dec/Alt drive training calibration.
Once you have calibrated and aligned your telescope, if you wish to start a new
model, go to the Smart Mount main menu. Locate and select "Erase" to clear the
current model.
Note: If you do not erase the current model, the training session will refine
the current model.
•Locate “Train” in the Smart Mount Configuration menu and press enter.
•The telescope will select and slew to several (over 40) stars.
•When requested to do so, carefully center each star and then press ENTER.
Next, proceed with the steps below:
OPTIONAL ACCESSORIES, pages 48 - 50 for more information.
illuminated reticle during the training procedure. An
If you find that you cannot see a star because there is an obstruction blocking your
view:
•Press MODE briefly to skip this star. Another star will be chosen.
To exit the training sequence before it is completed:
•Press and hold MODE for about two seconds and then release it.
When you have completed training:
•
Save your model, using a good, descriptive name, using the “Save As” menu.
Upon completion of the training, Smart Mount is enabled and
you choose “Off” from the Smart Mount Configuration menu.
remains on until
69
ermanently Mounted Scopes
P
For permanently mounted telescopes, it is not necessary to have more than one
model unless the weight and balance of auxiliary equipment introduces balance or
flexure changes that significantly affect pointing.The best practice is to train the Smart
Mount and then r
leave Smart Mount On as the installation default.
Other Menus Options
Save As and Load
The Smart Mount system allows you to save several models you have created (see
TRAINING on the previous page) using the Save As command. Choose which model
will be the "Current Model” using the Load command.
Update
The Update mode allows you to update training for the current model you have
enabled. You will sync on several stars as previously described, which will further
refine the pointing of your telescope. Save your model after running in update mode,
otherwise the update will be lost when the telescope is powered off.
On
Load a model from memory (see SAVE AS AND LOAD above) and then Select Smart
On. When Smart Mount is "On," the telescope will use the currently loaded model to
refine your telescope's pointing, but will not update the model (see
UPDATE above). If Smart Mount was "On" when you last powered off your telescope, it
will be "On" when you start the next session.
Off
When Smart Mount is "Off," the telescope will not use any model you have created to
refine pointing accuracy.
un a couple of sessions with Update enabled. Thereafter, simply
SMART MOUNT
Erase
The Erase command clears the Current Smart Mount table values to allow a new
model to be created.
Delete
The Delete command allows you to delete any model from memory. To delete a
model, just scroll through the names and select the model to you wish to delete and
press ENTER.You will be asked to confirm your choice. Press ENTER again and it will
be removed from memory.
70
Fig. 57: The Moon. Note the deep
shadows in the craters.
Fig. 58: The planet Jupiter. Jupiter's
four largest moons can be observed
in a different position every night.
Fig. 59: Saturn has the most extensive ring structure in our Solar
System.
BASIC ASTRONOMY
In the ear
RCX400, turned it skyward instead of looking at the distant trees and mountains. What
he sa
mankind thinks about the universe. Imagine what it must have been like being the first
human to see moons re
es of Venus! Because of his observations, Galileo correctly realized Earth's movement
and position around the Sun, and in doing so, gave birth to modern astronomy. Yet
Galileo's telescope was so crude, he could not clearly make out the rings of Saturn.
Galileo's discoveries laid the foundation for understanding the motion and nature of
the planets, stars, and galaxies. Building on his foundation, Henrietta Leavitt determined ho
possible origin of the universe, Albert Einstein unraveled the crucial relationship of
time and light, and 21st-century astronomers are currently discovering planets around
stars outside our solar system. Almost daily, using sophisticated successors to
Galileo's telescope, such as the Hubble Space Telescope and the Chandra X-Ray
Telescope, more and more mysteries of the universe are being probed and understood. We are living in the golden age of astronomy.
Unlike other sciences, astronomy welcomes contributions from amateurs. Much of the
knowledge we have on subjects such as comets, meteor showers, double and variable stars, the Moon, and our solar system comes from observations made by amateur astronomers. So as you look through your Meade
mind Galileo.To him, a telescope was not merely a machine made of glass and metal,
but something far more—a window of incredible discovery.
Autostar II Glossary
Be sure to make use of Autostar II’s Glossary feature. The Glossary menu provides
an alphabetical listing of definitions and descriptions of common astronomical terms.
Access directly through the Glossary menu or through hypertext words embedded in
Autostar II. See
Objects in Space
Listed below are some of the many astronomical objects that can be seen with your
RCX400:
The Moon
The Moon is, on average, a distance of 239,000 miles (380,000km) from Earth and is
best observed during its crescent or half phase when Sunlight strikes the Moon’s surface at an angle. It casts shadows and adds a sense of depth to the view (
No shadows are seen during a full Moon, causing the overly bright Moon to appear
flat and rather uninteresting through the telescope. Be sure to use a neutral Moon filter when observing the Moon. Not only does it protect your eyes from the bright glare
of the Moon, but it also helps enhance contrast, providing a more dramatic image.
Using your
of lunar craters and maria, described below.
Craters are round meteor impact sites covering most of the Moon’s surface. With no
atmosphere on the Moon, no weather conditions exist, so the only erosive force is
meteor strikes. Under these conditions, lunar craters can last for millions of years.
Maria (plural for mare) are smooth, dark areas scattered across the lunar surface.
These dark areas are large ancient impact basins that were filled with lava from the
interior of the Moon by the depth and force of a meteor or comet impact.
Twelve Apollo astronauts left their bootprints on the Moon in the late 1960's and early
1970's. However, no telescope on Earth is able to see these footprints or any other
ar
scope on Earth are about one-half mile across.
ly 17th century Italian Scientist Galileo, using a telescope smaller than your
w, and what he realized about what he saw, has forever changed the way
volve around the planet Jupiter or to see the changing phas-
w to measure the distance to stars, Edwin Hubble gave us a glimpse into the
RCX400 telescope, keep in
GLOSSARY MENU, page 31, for more information.
RCX400, brilliant detail can be observed on the Moon, including hundreds
. In fact, the smallest lunar features that may be seen with the largest tele-
acts
tif
Fig. 57).
71
Tip:
Enter a date in the Date
menu and you can determine if a planet(s) will be
visible during the night of
the entered date by checking its rise and set times.
Fig. 60: A favorite winter sight—the
great nebula in Orion.
Fig. 61: The Pleiades is one of the
most beautiful open clusters.
Fig. 62: The Andromeda Galaxy
largest galaxy of our local group.
, the
Planets
Planets change positions in the sky as they orbit around the Sun. To locate the planets on a given day or month, consult a monthly astronomy magazine, such as Sky andTelescope or Astronomy. You can also consult Autostar II for information about plan-
. Scroll to the "Object: Solar System" menu and scroll through the lists of planets.
ets
When a planet you are interested in displays, press ENTER. Use the Scroll keys to
display information about the planet, such as the planet's coordinates, and the rise
and set times. Listed below are the best planets for viewing through the
RCX400.
Venus is about nine-tenths the diameter of Earth. As Venus orbits the Sun, observers
can see it go through phases (crescent, half, and full) much like those of the Moon.
The disk of
Venus appears white as Sunlight is reflected off the thick cloud cover that
completely obscures any surface detail.
Mars is about half the diameter of Earth, and appears through the telescope as a tiny
reddish-orange disk. It may be possible to see a hint of white at one of the planet’s
polar ice caps. Approximately every two years, when Mars is closest to Earth in its
orbit, additional detail and coloring on the planet's surface may be visible.
Jupiter is the largest planet in our solar system and is 11 times the diameter of Earth.
Jupiter (
lines are cloud bands in the atmosphere
Fig. 58) appears as a disk with dark lines stretching across the surface.These
. Four of Jupiter’s moons (Io, Europa,
Ganymede, and Callisto) can be seen as “star-like” points of light when using even the
lowest magnification. These moons orbit Jupiter so that the number of moons visible
on any given night changes as they circle around the giant planet.
Saturn is nine times the diameter of Earth and appears as a small, round disk with
rings extending out from either side (Fig. 59). In 1610, Galileo, the first person to
observe Saturn through a telescope, did not understand that what he was seeing
were rings. Instead, he believed that Saturn had “ears.” Saturn’s rings are composed
of billions of ice particles ranging in size from a speck of dust to the size of a house.
The major division in Saturn's rings, called the Cassini Division, is easily visible
through the
RCX400. Titan, the largest of Saturn’s moons can also be seen as a bright,
star-like object near the planet.
Deep-Sky Objects
Star charts can be used to locate constellations, individual stars and deep-sky
objects. Examples of just some of the deep-sky objects you'll be able to observe with
RCX400 are given below:
your
Stars are large gaseous objects that are self-illuminated by nuclear fusion in their
core. Because of their vast distances from our solar system, all stars appear as pinpoints of light, irrespective of the size of the telescope used.
Nebulae are vast interstellar clouds of gas and dust where stars are formed. Most
impressive of these is the Great Nebula in Orion (M42) (
Fig. 60), a diffuse nebula that
appears as a faint wispy gray cloud. M42 is 1600 light years from Earth.
Open Clusters are loose groupings of young stars, all recently formed from the same
diffuse nebula.The Pleiades is an open cluster 410 light years away (Fig. 61).Through
the RCX400, numerous stars are visible.
Constellations are large, imaginary patterns of stars believed by ancient civilizations
to be the celestial equivalent of objects, animals, people, or gods. These patterns are
too large to be seen through a telescope. To learn the constellations, start with an
easy grouping of stars, such as the Big Dipper in Ursa Major. Then, use a star chart
to explore across the sky.
Galaxies are large assemblies of stars, nebulae, and star clusters that are bound by
gravity. The most common shape is spiral (such as our own Milky Way), but galaxies
can also be elliptical, or even irregular blobs. The Andromeda Galaxy (M31) (Fig. 62)
is the closest spiral-type galaxy to our own. This galaxy appears fuzzy and cigarshaped.
betw
It is 2.2 million light years away in the constellation Andromeda, located
.
een the large
of Cassiopeia and the g
“W”
reat square of P
egasus
72
MEADE LIMITED WARRANTY
Every Meade telescope, spotting scope, and telescope accessory is warranted by Meade Instruments Corporation (“Meade”)
to be free of defects in materials and workmanship for a period of ONE YEAR from the date of original purchase in the U.S.A.
and Canada. Meade will repair or replace a product, or part thereof, found by Meade to be defective, provided the defective
part is returned to Meade, freight-prepaid, with proof of purchase. This warranty applies to the original purchaser only and is
non-transferable. Meade products purchased outside North America are not included in this warranty, but are covered under
separate warranties issued by Meade international distributors.
RGA Number Required: Prior to the return of any product or part, a Return Goods Authorization (RGA) number must be
obtained from Meade b
detailing the nature of the claimed defect, as well as the owner’s name, address, and phone number.
This warranty is not valid in cases where the product has been abused or mishandled, where unauthorized repairs have been
attempted or performed, or where depreciation of the product is due to normal wear-and-tear. Meade specifically disclaims
special, indirect, or consequential damages or lost profit which may result from a breach of this warranty. Any implied warranties
which cannot be disclaimed are hereby limited to a term of one year from the date of original retail purchase.
This warranty gives you specific rights.You may have other rights which vary from state to state.
Meade reserves the right to change product specifications or to discontinue products without notice.
y writing, or calling (949) 451-1450. Each returned part or product must include a written statement
14-7600-00 3/05 B
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