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Finding the North Celestial Pole
In each hemisphere, there is a point in the sky around which all the other stars appear to rotate. These points are called the
celestial poles and are named for the hemisphere in which they reside. For example, in the northern hemisphere all stars move
around the north celestial pole. When the telescope's polar axis is pointed at the celestial pole, it is parallel to the Earth's
rotational axis.
Many methods of polar alignment require that you know how to find the celestial pole by identifying stars in the area. For those
in the northern hemisphere, finding the celestial pole is not too difficult. Fortunately, we have a naked eye star less than a degree
away. This star, Polaris, is the end star in the handle of the Little Dipper. Since the Little Dipper (technically called Ursa Minor)
is not one of the brightest constellations in the sky, it may be difficult to locate from urban areas. If this is the case, use the two
end stars in the bowl of the Big Dipper (the pointer stars). Draw an imaginary line through them toward the Little Dipper. They
point to Polaris (see Figure 5-5). The position of
the Big Dipper changes during the year and
throughout the course of the night (see Figure 5-4).
When the Big Dipper is low in the sky (i.e., near the
horizon), it may be difficult to locate. During these
times, look for Cassiopeia (see Figure 5-5).
Observers in the southern hemisphere are not as
fortunate as those in the northern hemisphere. The
stars around the south celestial pole are not nearly
as bright as those around the north. The closest star
that is relatively bright is Sigma Octantis. This star
is just within naked eye limit (magnitude 5.5) and
lies about 59 arc minutes from the pole.
The north celestial pole is the point in the
northern hemisphere around which all stars
appear to rotate. The counterpart in the
southern hemisphere is referred to as the south
celestial pole.
Polar Aligning the Mount
Latitude Scales
The easiest way to polar align a telescope is with a latitude scale. Unlike other methods that require you to find the celestial
pole by identifying certain stars near it, this method works off of a known constant to determine how high the polar axis
should be pointed. The CGE Pro mount can be adjusted from 15 to 65 degrees (see figure 5-3).
The constant, mentioned above, is a relationship between your latitude and
the angular distance the celestial pole is above the northern (or southern)
horizon; The angular distance from the northern horizon to the north
celestial pole is always equal to your latitude. To illustrate this, imagine
that you are standing on the north pole, latitude +90°. The north celestial
pole, which has a declination of +90°, would be directly overhead (i.e., 90
above the horizon). Now, let’s say that you move one degree south
your latitude is now +89° and the celestial pole is no longer directly
overhead. It has moved one degree closer toward the northern horizon.
This means the pole is now 89° above the northern horizon. If you move
one degree further south, the same thing happens again. You would have
to travel 70 miles north or south to change your latitude by one degree. As
you can see from this example, the distance from the northern horizon to
the celestial pole is always equal to your latitude.
Figure 5-3
Latitude
Scale
Latitude
Adjustment
Knob
Definition
Figure 5-5
The two stars in the front of the bowl of the Big Dipper point to Polaris which is less
than one degree from the true (north) celestial pole. Cassiopeia, the “W” shaped
constellation, is on the opposite side of the pole from the Big Dipper. The North
Celestial Pole (N.C.P.) is marked by the “+” sign.
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