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at the North Star, or Polaris. It lies within 1° of the north celes-
tial pole (NCP), which is an extension of the Earth's rotational
axis out into space. Stars in the Northern Hemisphere appear
to revolve around the NCP.
To find Polaris in the sky, look north and locate the pattern of
the Big Dipper (Figure 9). The two stars at the end of the "bowl"
of the Big Dipper point right to Polaris.
Observers in the Southern Hemisphere aren't so fortunate to
have a bright star so near the south celestial pole (SCP). The
star Sigma Octantis lies about 1° from the SCP, but it is barely
visible with the naked eye (magnitude 5.5).
For general visual observation, an approximate polar align-
ment is sufficient.
1. Level the equatorial mount by adjusting the length of the
three tripod legs.
2. There are two latitude adjustment L-bolts (see Figure 8);
loosen one while tightening the other. By doing this you will
adjust the latitude of the mount. Continue adjusting the
mount until the pointer on the latitude scale is set at the lati-
tude of your observing site. If you don't know your latitude,
consult a geographical atlas to find it. For example, if your
latitude is 35° North, set the pointer to 35. The latitude set-
ting should not have to be adjusted again unless you move
to a different viewing location some distance away.
Azimuth
adjustment
knobs
Figure 10.
For polar alignment, position the tripod so that the
"N" label at the base of the mount faces north. The azimuth fine
adjustment knobs above it are used to make small adjustments
to the mount's azimuth position. Be certain to loosen the tripod
attachment knob on the central support shaft before adjusting
these knobs.
3. Loosen the Dec. lock lever and rotate the telescope's optical
tube until it is parallel with the right ascension axis, as it is in
Figure 8.
4. Move the tripod so the telescope tube and right ascension
axis point roughly at Polaris. If you cannot see Polaris direct-
ly from your observing site, consult a compass and rotate
the tripod so the telescope points north. There is a label
bearing a large "N" at the base of the equatorial mount
(Figure 10); it should be facing north.
The equatorial mount is now polar aligned for casual observing.
More precise polar alignment is recommended for astropho-
tography. For this we suggest using the optional polar axis
finder scope.
From this point on in your observing session, you should not
make any further adjustments to the latitude of the mount, nor
should you move the tripod. Doing so will undo the polar align-
ment. The telescope should be moved only about its R.A. and
Dec. axes.
Eyepiece
Alignment
focus ring
setscrews (3)
Figure 11a.
The optional polar axis finder scope.
Figure 11b.
Installing the optional polar axis finder scope.
Polar alignment using an optional Polar axis
Finder scope
The SkyView Pro 80mm ED EQ mount can be equipped with
an optional polar axis finder scope (Figure 11a) which goes
inside the right ascension axis of the mount. The reticle of the
polar axis finder scope for the SkyView Pro has a tiny star map
printed on it. When properly aligned and used, it makes accu-
rate polar alignment quick and easy to do.
To install the polar axis finder scope, remove the cover at the
rear of the mount's right ascension axis and thread the polar axis
finder scope into the equatorial mount until tight (Figure 11b).
If you do not have a clear view of Polaris from your observing
site, you will not be able to use the polar-axis finder to pre-
cisely polar align the telescope. To align the mount using the
polar axis finder scope, follow these instructions:
1. Approximately polar-align the mount as outlined in the pro-
cedure previously.
2. Loosen the Dec. lock lever and rotate the optical tube on
the declination axis so that the tube is at a 90° to the right
ascension axis (Figure 12). Tighten the Dec. lock lever. This
Focus
Objective
lock-ring
lens
9
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