Obviously the scope needs to be balanced so that it moves freely (on the German equatorial [G.E.] mount) about both the R.A. and dec. axis (pl. form?), but I don't know much more than that. My instructional manual talks about how to balance the reflecting telescope in R.A. and in dec. (though I could use a little clarification on their instructions) but it does NOT explain why you would put the telescope in either of these positions. I understand that R.A. involves moving the scope around the polar axis, and declination allows you move away from the center of the sky's rotation (practically centered on Polaris) to any star in the sky, except when the tripod gets in the way. How do we balance the scope in each position, and why do we choose one over the other?
Bonus question: With a smaller weight and a larger weight, how are each used in the balancing process and is it okay to switch the weights with the scope still attached to the mount?
2007-05-19
11:11:39
·
2 answers
·
asked by
Andy
4
in
Science & Mathematics
➔ Astronomy & Space