mreq
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mreq said:I want to know how that point on the orbit it's calculated.
Because i set the time to june 10th 1564 (location randomly) and the sun it's in taurus constelation.
Thanks!
mreq said:Skyglobe seems to be old!
Isn't there any software to be truly profesional ? What's so hard ? (i mean like there is movie editor - which do everything ...it should be a astronomy software...)
Janus said:We already covered that back in post #30. The Sidereal year is 365 days, 6 hr, 9 min, 9.7676 sec long. Thus in a non-leap year. the Earth will be 6 hr, 9 min, 9.7676 sec short of a complete orbit the next Feb 19. This works out to just about 1/4 of a degree or half the width of the Moon.
However, during a leap year, which is 366 days long, the year is longer than it takes for the Earth to complete an orbit by some 3/4 of a degree. So what you would get is the Earth falling behind by 1/4 of a degree for each of 3 years and then making that up in the fourth year. There will still be a minor drift caused by the difference between Tropical and sidereal year (again, as noted in post 30), but this would take years to notice.
Integral said:This last bit of drift is compensated for with the century leap years, that is a century year (1800, 1900 etc. ) is NOT a leap year even though it is obvioulsy a multiple of 4, unless it is still divisible by 4 after dividing by 100. Thus the year 2000 was a leap year making it part of a 400 year correction cycle. I somehow feel cheated because the rare event that occurred in 2000 meant that we maintained the leap year cycle that we have all become familiar with. Since the current calendar system was established in the 1750's this is the first century which was a leap year.