This booklet has been written as an introduction to your new Davis sextant. By
studying its pages, you will learn how to operate your sextant, how to find the altitude of the sun, and how to use your readings to calculate location. The meridian
transit method of navigation described is both easily learned and simply
applied. When you finish reading, the mystery surrounding celestial navigation
and sextant use should disappear. Before becoming an accomplished navigator,
however, you will need to study those aspects of navigation which are beyond the
scope of this booklet.
HOW TO READ THE VERNIER
There are two scales on the sextant. The scale on the frame is called the “arc,”
while the scale on the index arm is the “vernier.” Each division of the arc equals
one degree. Each division of the vernier equals two minutes (2'). To read the
number of degrees, find the lines on the arc which are closest to the zero mark on
the vernier. The zero mark is usually somewhere between two lines. The correct
arc reading is always that of the lower value, i.e., the line to the right of the zero
mark. To read fractions of a degree, find the division of the vernier which is in
alignment with a division of the arc.
To get a clear picture of how this works, set the zero on the vernier exactly
beneath any whole degree mark on the arc—letʼs say 30°. Now move the index
arm very slightly to the left until the first vernier mark to the right of the zero lines
up exactly with a mark on the arc. Since the marks on the vernier are 2' apart,
you have actually moved the index arm 2' beyond 30°; your sextant reads 30° 02'.
Now, move the index arm slightly further to the left so that the next division of the
vernier comes into alignment with a division of the arc. Your sextant now reads
30° 04' (Fig. 1).
As you continue moving the index arm, successive divisions of the vernier will
come into alignment with a division of the arc. When the last mark on the vernier
(60') is in alignment with a division of the arc, the sextant will read 31°. In figure 2
below, the sextant reads 43° 26'.
Figure 1
Figure 2
Page 1
MARK 3 SEXTANT ADJUSTMENT
Adjusting your Mark 3 Sextant is easy and should be done each time it is used.
All adjustments are made with the index mirror, the large movable mirror at the
pivot of the index arm (it is not necessary to adjust the small horizon mirror, as
the unit construction makes it impossible to be very much in error). On a correctly
adjusted sextant, the index mirror is perpendicular to the frame and becomes parallel to the horizon mirror when the sextant reads zero.
First, adjust the index mirror for “side error” by making it perpendicular to the
frame. Holding the sextant in your right hand, raise the instrument to your eye.
Look at any horizontal straight edge (the sea horizon, for example, or the roof of a
building al least one mile away) and move the index arm back and forth. The real
horizon will remain still while the mirror horizon will appear only when the scales
read close to zero. Line up the mirror horizon and the real horizon so that both
appear as a single straight line (fig. 3).
Mirror horizon is not aligned with
the real horizon—index arm is not
in proper position.
Mirror horizon and real horizon
form a single straight line—index
arm is properly positioned.
Figure 3
Now do a vertical adjustment. Without changing the setting, look through the
sextant at any vertical line (a flag pole, for example, or the edge of a building) and
swing the instrument back and forth across the vertical line. If the index mirror is
not perpendicular to the frame, the line will seem to jump to one side as the mirror
passes it. To correct this, slowly tighten or loosen the screw closest to the frame at
the back of the index mirror until the vertical line no longer appears to jump (fig. 4).
Index mirror screw
too tight.
Index mirror screw
correctly adjusted.
Index mirror screw
too loose.
Figure 4
Page 2
Finally, remove the index error. Set the sextant at zero and look at the horizon.
With the sextant still held to your eye, turn the screw that is furthest from the frame
at the back of the index mirror until the two horizons move together and form one
straight line. The index mirror is now parallel to the horizon mirror (Fig. 5).
Index mirror not parallel to
horizon mirror.
On a correctly adjusted sextant, the real and mirror horizons remain in a single
line when the instrument is rocked from side to side (Fig. 6).
Figure 5
Index mirror parallel to
horizon mirror.
Figure 6
While you should know how to adjust your sextant for index error, it is not necessary to remove it entirely. It is standard practice to simply note the error and then
correct oneʼs reading for this amount each time the sextant is used (as much as
6' index error is allowable). To check for index error, hold the sextant in your right
hand and look at the sea horizon. By moving the index arm, line up the real and
mirror horizons so that both appear as a single straight line. Now, look at the
scale. If it reads zero, there is no index error. If the scale reads anything but zero,
there is an index error which must be added to or subtracted from each reading.
For example, if the scale reads +6' when the horizons are aligned, the 6ʼ is subtracted. If the reading is below the zero mark, for example –6', the 6' is added
(Note: for an index error of –6', the scale actually reads 54').
MEASURING THE SUN’S ALTITUDE
When looking at the sun through the sextant, be sure to use a sufficient number of shades to protect your eyes from the direct rays of the sun. Choose
the combination of index and horizon shades that gives you a clear image of the
sun without glare.
Page 3
To measure the sun’s altitude, stand facing the sun with the sextant in your
right hand. With your left hand on the index arm, look through the eye piece at the
horizon and move the index arm until the sun is visible through the two mirrors
and index shades. Rock the entire sextant from side to side so that the sunʼs
image travels in a half-arc. Now, adjust the index arm to bring the sunʼs image
down to just touch the horizon (Fig. 7).
Figure 7
The sun’s image travels
in a short arc which just
touches the horizon.
Being careful not to disturb the setting, read the sunʼs altitude from the scales on
the sextant. Since all calculations in the Navigation Tables use the center of the
sun or moon, this lower limb reading must be adjusted for semi-diameter correction, shown later.
HEIGHT OF EYE
When measuring the altitude of the sun, we want to measure the angle formed by
a ray from the sun and a plane tangent to the earth at the point where the observer is standing. Due to the height of the eye of the observer, however, the visible
horizon actually falls below this theoretical plane (Fig. 8).
To correct for the height of
the eye, one must apply a
“dip correction.” Dip correc-
tion increases as the eye is
raised further above the surface of the water (Table 1)
and must always be subtracted from the sextant reading.
Table 1
Height of Eye Correction
Feet Meters Dip
5 1.5 2'
10 3.0 3'
15 4.5 4'
25 7.5 5'
40 12.0 6'
Page 4
Figure 8
Due to the height of the eye of the observer, the
visible horizon (H) falls below the plane (P) tan-
gent to the earth at the point where the observer
is standing.
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