Abstract
The Saros cycle has been known since antiquity and refers to the periodicity of eclipses. It is the least common multiple of three periods: the synodic, the draconic, and the anomalistic months. We show how to obtain these periods from Newton's laws with a precision greater than 0.02% using only the sidereal month and year as references.
Original language | English |
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Article number | 1303 |
Journal | Revista Brasileira De Ensino De Fisica |
Volume | 31 |
Issue number | 1 |
DOIs | |
Publication status | Published - Mar 2009 |
Keywords
- eclipses
- Newton's laws
- Restricted 3-body problem
- Saros cycles