Physics
Scientific paper
Jun 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006o%26t....62...23s&link_type=abstract
Observations & Travaux, vol. 62, p. 23-25
Physics
Scientific paper
As the method of Kepler to determine the orbit of Mars is well known, his method concerning that of the Earth is much less popular. Kepler obtained a very precise orbit of the Earth from only four well-chosen longitudes of the Sun and of Mars. By trial and error, the orbit was found a circular one, with an eccentricity of 0,01653, the longitude of the perihelion being 100&°19'.
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