a. |
| b. |
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c. |
| d. |
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Figure 10. This illustration shows the telescope pointed in the four cardinal directions: (a) north, (b) south, (c) east, (d) west. Note that the tripod and mount have not been moved; only the telescope tube has been moved on the R.A. and Dec. axes.
Figure 10 illustrates how the telescope will look when pointed at the four cardinal
The key things to remember when pointing the telescope are that a) you only move it in R.A. and Dec., not in azimuth or lat- itude (altitude), and b) the counterweight and shaft will not always appear as it does in Figure 1. In fact it almost never will!
6.Using Your Telescope— Astronomical Observing
Choosing an Observing Site
When selecting a location for observing, get as far away as possible from direct artificial light such as streetlights, porch lights, and automobile headlights. The glare from these lights will greatly impair your
If at all possible, escape the
Cooling the Telescope
All optical instruments need time to reach “thermal equilibri- um.” The bigger the instrument and the larger the temperature change, the more time is needed. Allow at least a
Aiming the Telescope
To view an object in the main telescope, first loosen both the R.A. and Dec. lock levers. Aim the telescope at the object you wish to observe by “eyeballing” along the length of the telescope tube (or use the setting circles to “dial in” the object’s coordinates).Then look through the (aligned) finder scope and move the telescope tube until the object is generally centered on the finder’s crosshairs. Retighten the R.A. and Dec. lock levers.Then accurately center the object on the finder’s crosshairs using the R.A. and Dec. slow- motion controls. The object should now be visible in the main telescope with a
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