Astronomical algorithm: Difference between revisions
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'''Astronomical algorithms''' are the [[algorithm]]s used to calculate [[ephemeris|ephemerides]], [[calendar]]s, and positions (as in [[celestial navigation]] or [[satellite navigation]]). Examples of large and complex [[astronomy|astronomical]] algorithms are those used to calculate the position of the [[Moon]]. A simple example is the [[Julian day#Calculation|calculation of the Julian day]]. |
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[[Numerical model of solar system]] discusses a generalized approach to local astronomical modeling. The ''[[variations séculaires des orbites planétaires]]'' describes an often used model. |
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== See also == |
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* [[Astrodynamics]] |
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* [[Celestial mechanics]] |
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* [[Charge-coupled device]] (a data-collecting device that is sometimes aimed at the sky and requires algorithms to process its output) |
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* [[Doomsday rule]] |
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* [[List of astronomical objects]] |
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* [[Jean Meeus|Meeus, Jean]] |
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* [[Transformation from spherical coordinates to rectangular coordinates]] |
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* [https://web.archive.org/web/20070105005127/http://www.sunlit-design.com/products/thesunapi/documentation/funcref.php?indexref=4 An implementation of Astronomical Algorithms. Calculate MJD, Equation of Time and Solar Declination in Excel, CAD or your other programs.] The Sun API is free and extremely accurate. For Windows Computers. |
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* [https://web.archive.org/web/20150227205958/http://www.astronomyapi.com/ astronomy API] An API to the Universe |
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[[Category:Astrodynamics]] |
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[[Category:Computational physics]] |
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[[Category:Calendar algorithms]] |
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Latest revision as of 20:28, 12 October 2020
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