Figure 6. The equatorial mount of the StarMax 127mm EQ
Declination setting circle
Front opening in R.A. axis
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Azimuth
fine adjustment knobs
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Declination locking lever
Right ascension locking lever
Right ascension setting circle
Polar axis finder scope Latitude scale
Latitude adjusting
To find Polaris in the sky, look north and locate the pattern of the Big Dipper (Figure 7). 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 altitude adjusting
3.Loosen the Dec. lock lever and rotate the telescope optical tube until it is parallel with the R.A. axis, as it is in Figure 1. The pointer on the Dec. setting circle should read 90°. Retighten the Dec. lock lever.
4.Move the tripod so the telescope tube (and R.A. axis) points roughly at Polaris. If you cannot see Polaris directly 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
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Figure 7. To find Polaris in the night sky, look north and find the Big Dipper. Extend an imaginary line from the two "Pointer Stars" in the bowl of the Big Dipper. Go about five times the distance between those stars and you'll reach Polaris, which lies within 1° of the north celestial pole (NCP).
the base of the equatorial mount (Figure 8). It should be fac- ing north.
The equatorial mount is now polar aligned for casual observ- ing. More precise polar alignment is recommended for astrophotography.
From this point on in your observing session, you should not make any further adjustments in the azimuth or the latitude of the mount, nor should you move the tripod. Doing so will undo the polar alignment. The telescope should be moved only about its R.A. and Dec. axes.
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