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I (Brian Tung) wrote:
The Earth's orbit, however, is only slightly elliptical. Its distance from the Sun varies only by a little more than 3 percent throughout the year. The variation in the Sun's apparent motion doesn't change very much as a result (about 6 percent, twice the variation in distance)[*], and its effect is never so great as to ever be *greater* than the rotational motion (which, after all, is 366 times greater on average). Generally speaking, we just don't notice. That is *not* the case with Mercury. First of all, its orbit is much more elliptical than the Earth's. Its distance from the Sun varies by some 40 percent, and the Sun's apparent motion, as seen from Mercury, therefore varies by almost a factor of 2[*]. [*] In both the cases, I mean the apparent motion *due solely to the planet's orbital motion*. Sorry about any possible confusion. Brian Tung The Astronomy Corner at http://astro.isi.edu/ Unofficial C5+ Home Page at http://astro.isi.edu/c5plus/ The PleiadAtlas Home Page at http://astro.isi.edu/pleiadatlas/ My Own Personal FAQ (SAA) at http://astro.isi.edu/reference/faq.txt |
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