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Sun transit time question May 5, 2004
Posted by E.D.G. May 5, 2004 I am working with a professional computer programmer to develop Basic and Perl language programs which will generate subsolar and sublunar point latitudes and longitudes. The first program is now running and is being "fine tuned." In developing it I noticed something and am curious regarding what causes it. Perhaps someone reading this note will know the answer. In theory the sun should be directly above 0 longitude, the Greenwich longitude, at 12 noon each day. But the longitude numbers for its actual location at 12 noon that this and other programs generate show that there is a variation of perhaps as much as 15 minutes in that transit time at different times of the year. And those variations are reproducible from year to year. Q: What is the cause of those variations? I am assuming that I am interpreting the data correctly. Might this be due to the fact that the Earth orbit is an ellipse rather than a true circle. And for that reason the 0 longitude line is directly beneath the sun at slightly different times during the year because the Earth rotation does not perfectly match its constantly changing orbital speed around the sun? |
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