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Newbie question. After a couple of hours of binocular study of Auriga,
I sat down with Burnhams and Uranometria 2000 to identify the things I'd seen (lots of surprises in Auriga if you haven't looked before - it was great fun, even though I had to peek through gaps in clouds to get a view). While poring over the books, I discovered something puzzling. There's an apparent 4 minute RA discrepancy between objects plotted in U2000 and positions given in Burnhams? Dec is OK, but everything is moved over by 1 grid in U2000. They can't BOTH be right! What gives? Or am I reading U2000 wrong? Thanks Beats |
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I would imagine it's because the coordinates given in Burnhams are
Epoch 1950.0. Scotty On 9 Oct 2003 00:30:59 -0700, (justbeats) wrote: Newbie question. After a couple of hours of binocular study of Auriga, I sat down with Burnhams and Uranometria 2000 to identify the things I'd seen (lots of surprises in Auriga if you haven't looked before - it was great fun, even though I had to peek through gaps in clouds to get a view). While poring over the books, I discovered something puzzling. There's an apparent 4 minute RA discrepancy between objects plotted in U2000 and positions given in Burnhams? Dec is OK, but everything is moved over by 1 grid in U2000. They can't BOTH be right! What gives? Or am I reading U2000 wrong? Thanks Beats |
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justbeats wrote:
Newbie question. After a couple of hours of binocular study of Auriga, I sat down with Burnhams and Uranometria 2000 to identify the things I'd seen (lots of surprises in Auriga if you haven't looked before - it was great fun, even though I had to peek through gaps in clouds to get a view). While poring over the books, I discovered something puzzling. There's an apparent 4 minute RA discrepancy between objects plotted in U2000 and positions given in Burnhams? Dec is OK, but everything is moved over by 1 grid in U2000. They can't BOTH be right! What gives? Or am I reading U2000 wrong? Thanks Beats Precession of the Equinoxes http://scienceworld.wolfram.com/phys...Equinoxes.html Burnham's Celestial Handbook is based on epoch 1950.0 Uranometria 2000.0 uses equinox 2000.0. Uranometria 2000.0's stellar data base was augmented to include the 50 nearest stars and the 25 greatest proper motion stars no matter how faint. Those stars' positions known in 1950.0 coordinated were processed to equinox 2000.0. |
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![]() "justbeats" wrote in message m... Newbie question. After a couple of hours of binocular study of Auriga, I sat down with Burnhams and Uranometria 2000 to identify the things I'd seen (lots of surprises in Auriga if you haven't looked before - it was great fun, even though I had to peek through gaps in clouds to get a view). While poring over the books, I discovered something puzzling. There's an apparent 4 minute RA discrepancy between objects plotted in U2000 and positions given in Burnhams? Dec is OK, but everything is moved over by 1 grid in U2000. The positions in Uranometria are for epoch 2000; those of Burnham, 1950. The epoch of a position is the date (year) for which the r.a. and declination are calculated. Because of precession (a steady change in the direction of the earth's axis), R.A. and declination are constantly changing all over the sky. The rate of change is about 3/4 degree per century, if I recall correctly. -- Clear skies, Michael Covington -- www.covingtoninnovations.com Author, Astrophotography for the Amateur and (new) How to Use a Computerized Telescope |
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