Meade LX10 Manual de usuario Pagina 6

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4.3.4 How to Use a Planisphere
1. Note the d a t e and tim e (if the clocks are set for d aylight savings time, deduct an hour
from your clock tim e) .
2. On the sky wheel, tu r n the wheel unt i l it matches your time and date. The elliptical-
shaped opening shows t h e visible stars.
Figure 4.5: Finding Polaris
3. Find North. Hold the planisphere such that North is at the bottom. The hole in the
center marks t h e location of Polaris, the North star. (To find Polaris in the sky at
night, first l ocate the Big Dip per. The two stars at the end of the ‘spoon’ point to
Polaris. Refer to Figure 4.5.)
4. The planisphere is a projection of the night sky. Hold the pl a n i sp h er e up; it should
correspond to what the sky looks like. The stars directly overhead will be found in the
center of the map and those to t h e north will be at the bottom. The reverse side of
the planisphere shows the stars to t h e south. Always hold the pl an i sp h er e so that the
direction you are facing is at the bottom. Alternati vely, you may find that it is easier
to use the chart wh en lying down.
Notice how the planisphere marks t h e celestial coordinates. Declination i s shown as a series
of concentric circles, with 90 being in the center. RA is sh own as a series of spokes, radiating
from the center. Recall how we can u se RA to determine at what time a star will be directly
overhead.
These small charts can be misleading in s everal r espects. This is not due to any flaw in their
design; it is simply due to the fact that they are trying to capture a large hemisphere of the
sky and represent it on a small flat circle. Firstly, the angular scale of objects in the sky is
much larger than on the map. The h ar d est part in usin g such a chart is making the transfer
from a small area on the map to a large are a on the sky. You can see the entire chart at
once but you cannot see the entire sky at once.
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