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he easiest way to polar align a telescope is with a latitude scale. Unlike other methods that require you to find the
this example, the distance from the northern horizon to the celestial
pole is always equal to your latitude.
If you are observing from Los Angeles, which has a latitude of 34°,
a
cope at
. To
Figure 4-3
1. ake sure the polar axis of the mount is pointing due north. Use a landmark that you know faces north.
2. evel the tripod. There is a bubble level built into the mount for this purpose.
OTE: Leveling the tripod is only necessary if using this method of polar alignment. Perfect polar alignment is still
ossible using other methods described later in this manual without leveling the tripod.
3. djust the mount in altitude until the latitude indicator points to your latitude. Moving the mount affects the angle the
olar axis is pointing. For specific information on adjusting the equatorial mount, please see the section “Adjusting the
ount.”
his method can be done in daylight, thus eliminating the need to fumble around in the dark. Although this method
oes NOT put you directly on the pole, it will limit the number of corrections you will make when tracking an object.
will also be accurate enough for short exposure prime focus planetary photography (a couple of seconds) and short
xposure piggyback astrophotography (a couple of minutes).
T
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 Omni CG-4 mount can be adjusted from about 20 to 60 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
then the celestial pole is 34° above the northern horizon. All
latitude scale does then is to point the polar axis of the teles
the right elevation above the northern (or southern) horizon
align your telescope:
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his method utilizes Polaris as a guidepost to the celestial pole. Since Polaris is less than a degree from the celestial
ole, you can simply point the polar axis of your telescope at Polaris. Although this is by no means perfect alignment,
does get you within one degree. Unlike the previous method, this must be done in the dark when Polaris is visible.
1. et the telescope up so that the polar axis is pointing north.
2. oosen the DEC clutch knob and move the telescope so that the tube is parallel to the polar axis. When this is done,
e declination setting circle will read +90°. If the declination setting circle is not aligned, move the telescope so that
e tube is parallel to the polar axis.
3. djust the mount in altitude and/or azimuth until Polaris is in the field of view of the finder.
4. enter Polaris in the field of the telescope using the fine adjustment controls on the mount.
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