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 at or near the Sun. Do not look through the
telescope or SmartFinder™as it is moving. Children
should always have adult supervision while observing.
INTRODUCTION
Your telescope is an excellent beginner’s
instrument, and is designed to observe
objects in the sky and also on land. It can be
your personal window on the universe or
allows you to intimately study the behavior of
nesting birds on a distant hillside.
The telescope is shipped with the following
parts:
• Optical tube
• Aluminum tripod with an accessory tray
• Two 1.25" eyepieces: MA25mm (28X),
MH9mm (78X)
• 2x 1.25" Barlow lens
• Diagonal mirror
• Red dot viewfinder with bracket
• Telescope mount
The tube has a focal length of 700mm, and
its objective lens has a diameter of 60mm.
The lens diameter is one of the most
important pieces of information about the
telescope. The size of the objective lens
determines how much detail you will be able
to see in your telescope. The focal length will
help later on to calculate magnification.
Setting up your telescope involves these
simple steps:
• Assemble your tripod
• Attach the accessory tray
• Attach the optical tube to the mount
• Attach the red dot viewfinder
• Attach the diagonal mirror and eyepiece
• Align the red dot viewfinder
Study the the picture on the next page and
become acquainted with the parts of your
telescope. Then proceed to “Assemble
your Tripod.”
1
FIGURE 1
2
1. Eyepiece
2. Red dot viewfinder (see Inset A)
3. Red dot viewfinder alignment screws
(see Inset A)
4. Optical tube assembly
5. Vertical locking lever
6. Horizontal lock knob
7. Tripod legs
8. Leg brace supports (See Inset C)
9. Leg brace (See Inset C)
10. Mount base attachment
11. Optical tube lock knobs
12. Horizontal slow motion controll (See Inset B)
13. Diagonal mirror
14. Objective lens cell
15. Focuser drawtube
16. Vertical slow motion control (See Inset B)
17. Accessory tray (Inset C)
18. Red dot viewfinder bracket (see Inset A)
19. Adjustable sliding leg extension (see Inset C)
Inset A:Red Dot Viewfinder Assembly
Inset B:Tripod Legs and Accessory Tray
Inset C:Altaz or Azimuth Mount
(Not visible)
Inset A
Inset B
Inset C
ASSEMBLE YOUR TRIPOD
The tripod is the basic support for your
telescope. Its height may be adjusted so
that you can view comfortably.
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ttooFFiigg..11..
1. Spread the legs out evenly apart.
2. Set the height of your tripod unlock the leg
lock (20).
3. Slide leg (19) in or out to the desired
length
Inset B
4. Tighten the leg
Fig. 2
lock. See Inset B.
3. Rotate the tray, locking the corners of the
tray in place on the leg brace supports.
ATTACH THE RED DOT VIEWFINDER
An eyepiece (1) has a narrow field of
view. A viewfinder (2) has a wider field
of view, which makes it easier to locate
objects. The red dot viewfinder has a red dot
to make it easier to line up more precisely
with a target.
1. Note the red dot viewfinder (2) has a
quick release mounting bracket (18).
2. Slide the red dot viewfinder (2) into the
Fig. 3
lock (20) to
relock the leg
lock.
5. Repeat for the
other two legs.
ATTACH TH E
ACCESSORY TRAY
The tray helps stabilize the tripod and is also
a convenient holder of eyepieces and other
Meade accessories, such as the Barlow lens.
1. Place the accessory tray (17) over the
center of the leg brace supports (8).
2. Rotate the tray so it fits onto the central
Looking at or near the Sun will cause irreversible damage to your eye. Do not point this telescope at or near the Sun. Do not look through the telescope as it is moving.
ATTACH THE OPTICAL TUBE TO THE MOUNT
The optical tube gathers distant light which
is focused in the eyepiece.
1. Remove the two lock knobs (11) from the
optical tube.
2. Slide the altitude rod into the hole in the
altitude adjustment control. Tighten to a
firm feel. See Fig. 2.
3. Place the optical tube (4) onto the
mounting bracket Fig. 2.
4. Thread a lock knob (11) onto each of the
mounting screws and tighten to a firm
feel. See Fig. 2.
ATTACH THE DIAGONAL MIRROR AND
EYEPIECE
The diagonal mirror reflects the light from
the optical tube to a more comfortable
viewing position.
1. Slide the diagonal mirror (13) into the
focuser drawtube(15).
mounting bracket as shown on Fig. 3.
NNoottee::
To detach
the bracket
press the
bracket quick
release button
and slide the
bracket out.
3
2. Tighten the drawtube thumbscrew to
hold the diagonal mirror securely.
4
3. Slide the MA 25mm eyepiece (1) into
diagonal mirror (13).
4. Tighten the diagonal mirror thumbscrew
(26) to hold the eyepiece securely.
ALIGN THE RED DOT VIEWFINDER
Perform the first part of this procedure
during the daytime and the last step at night.
1. Point the telescope at an easy-to-find
land object such as the top of a telephone
pole or a distant mountain or tower. Look
through the eyepiece in the diagonal
mirror and turn the focuser knob (23)
until the image is sharply focused. Center
the object precisely in the eyepiece’s field
of view.
2. Look through the red dot viewfinder. Turn
one or more of the viewfinder’s alignment
screws (3) until the red dot is precisely
over the same object as you centered in
the eyepiece.
3. Check this alignment at night on a
celestial object, such as the Moon or
a bright star, and use the viewfinder’s
Looking at or near the Sun will cause irreversible damage to your eye. Do not point this telescope at or near the Sun. Do not look through the telescope as it is moving.
alignment screws to make any
necessary refinements.
TO MOVE THE TELESCOPE
Your telescope is altazimuth mounted.
Altazimuth is just a complicated way of saying
that your telescope moves up and down and
from side to side. Other telescopes may be
mounted in different ways.
1. Slightly loosen the vertical locking lever
(5). Loosening this lever allows you to
move the telescope up and down.
2. Slightly loosen the horizontal lock knob (6).
Loosening this lock allows the telescope to
be moved from side to side.
3. Once an object is found, re-tighten the
knob. You can then use the slow motion
controls to make smooth and precise
movements as you follow (or “track”) an
object as it moves in the eyepiece.
You will enjoy your telescope even more as
you learn more about it. But don’t be scared
off by difficult terms or complicated
procedures. Don’t panic! Just relax and enjoy
your scope.
THE MOST IMPORTANT RULE
We have one very important rule that
you should always follow when using
your telescope:
Have a good time when you’re observing. You
may not know everything that there is to
know about a telescope or what all the
sights in the universe are, but that’s OK. Just
point and observe at first.
You will begin to grow and learn more about
astronomy the more you observe. Go to the
Have Fun!
library and read some books about the stars
and planets. Read about astronomers of
old. Many of them had telescope no bigger
than the one you are using right now.
Galileo, who is one of the first astronomers
to use a telescope, discovered four of the
moons of Jupiter with a telescope about the
same size as yours (and his didn’t even
focus very well!).
OBSERVING
Observe during the daytime: Try out your
telescope during the daytime at first. It is
easier to learn how it operates and how to
observe when it is light.
Pick out an easy object to observe: A distant
mountain, a large tree, a lighthouse or
skyscraper make excellent targets. Point the
optical tube so it lines up with your object.
Unlock the lock knobs: To move the
telescope, you will need to unlock the
horizontal lock knob (6) and vertical locking
lever(5) (just rotate to unlock or lock; when
locking, only tighten to a “firm feel,” do not
overtighten).
Looking at or near the Sun will cause irreversible damage to your eye. Do not point this telescope at or near the Sun. Do not look through the telescope as it is moving.
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.
Use the red dot viewfinder: If you have not
done so, align the viewfinder (2) with the
telescope’s eyepiece (1) as described earlier.
Look through the viewfinder until you can
see the object. It will be easier to locate an
object using the viewfinder rather than
locating with the eyepiece. Line up the object
with the viewfinders red dot.
Look through the eyepiece: Once you have
the object lined up in the viewfinder, look
through the optical tube’s eyepiece. If you
have aligned your viewfinder, you will you
see the object in your eyepiece.
SSUUNNWWAARRNNIINNGG
NEVER USE YOUR TELESCOPE
TO LOOK AT THE SUN!
Focus: Look through the eyepiece and
practice focusing on the object you
have chosen.
Try out the slow motion adjustment
controls: Practice using the slow motion
controls (12 and 16) to move the telescope.
These can come in very handy, especially
when you wish to move the telescope in very
small (fine control) steps.
Observe the Moon: When you feel
comfortable with the viewfinder, the
eyepieces, the locks and the adjustment
controls, you will be ready to try out the
telescope at night. The Moon is the best
object to observe the first time you go out at
night. Pick a night when the Moon is a
You haven’t just bought a telescope, you have embarked
on an astronomy adventure that never ends. Share the
journey with others by accepting your free membership
in the 4M community of astronomers.
Go to www.Meade4M.org to activate your membership
today.
5
THE MEADE 4M COMMUNITY
crescent. No shadows are seen during
a full Moon, making it appear flat
6
and uninteresting.
Look for different features on the Moon. The
most obvious features are craters. In fact
you can see craters within craters. Some
craters have bright lines about them. These
are called rays and are the result of material
volcanic activity. You can also see mountain
ranges and fault lines on the Moon.
Use a neutral density filter (often called a
“moon filter”) when observing the Moon.
Neutral density filters are available from
Meade as an optional accessory and
enhance contrast to improve your
observation of lunar features.
is a single, yellow dwarf star. It is average as
far as stars go and is a middle aged star.
Beyond the planets are clouds of comets, icy
planetoids and other debris left over from
the birth of our sun. Recently astronomers
have found large objects in this area and
they may increase the number of planets in
our solar system.
thrown out of the crater when it was struck
by a colliding object. The dark areas on the
Moon are called maria and are composed of
lava from the period when the Moon still had
TOO MUCH POWER?
Can you ever have too much power? If the type of
power you’re referring to is eyepiece magnification,
yes you can! The most common mistake of the
beginning observer is to “overpower” a telescope
by using high magnifications which the telescope’s
aperture and atmospheric conditions cannot
reasonably support. 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.
Powers above 400x should be employed only under
the steadiest atmospheric conditions.
Spend several nights observing the Moon.
Some nights, the Moon is so bright that it
makes other objects in the sky difficult to
see. These are nights that are excellent for
lunar observation.
Observe the Solar System: After observing
the Moon, you are ready to step up to the
next level of observation, the planets.
There are four planets that you can easily
observe in your telescope: Venus, Mars,
Jupiter and Saturn.
Nine planets (maybe more!) travel in a fairly
circular pattern around our Sun. Any system
of planets orbiting one or more stars is
called a solar system. Our Sun, by the way,
The four planets closest to the Sun are rocky
and are called the inner planets. Mercury,
Venus, Earth and Mars comprise the inner
planets. Venus and Mars can be easily seen
in your telescope.
Venus is seen before dawn or after sunset,
because it is close to the Sun. You can
observe Venus going through crescent
phases. But you cannot see any surface
detail on Venus because it has a very thick
atmosphere of gas.
When Mars is close to the Earth, you can see
some details on Mars, and sometimes even
Mars’ polar caps. But quite often, Mars is
further away and just appears as a red dot
with some dark lines crisscrossing it.
Looking at or near the Sun will cause irreversible damage to your eye. Do not point this telescope at or near the Sun. Do not look through the telescope as it is moving.
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