The unitary S-code description of the one-body Kepler problem is shown to unfold naturally from a primigenial sphere (with centre at the attracting gravitational centre and radius related to the universal constant of gravitation). In this spherical scenery all the Kepler problem fundamental elements are recovered by simple linear vector combinations.
The Kepler problem primigenial sphere
VIVARELLI, MARIA DINA
2015-01-01
Abstract
The unitary S-code description of the one-body Kepler problem is shown to unfold naturally from a primigenial sphere (with centre at the attracting gravitational centre and radius related to the universal constant of gravitation). In this spherical scenery all the Kepler problem fundamental elements are recovered by simple linear vector combinations.File in questo prodotto:
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