On the classical expansion of the perturbing function in individual orbital elements

Details On the classical expansion of the perturbing function in individual orbital elements On the classical expansion of the perturbing function in individual orbital elements

Jul 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999cemda..74..147t&link_type=abstract

Celestial Mechanics and Dynamical Astronomy, v. 74, Issue 3, p. 147-152 (1999).

Astronomy and Astrophysics

Astronomy

Asteroid Motion, Perturbing Function, Asteroid Proper Elements, Asteroid Motion, Perturbing Function, Asteroid Proper Elements

Scientific paper

Starting from the classical expansion of the perturbing function in the three-body problem, the transformation to individual orbital elements is performed in principle up to any degree in small parameters. Some corrections to the results presented in the well-known article by Yuasa on secular perturbations of asteroids are given. Consequences for the expansion of the indirect part of the perturbing function are discussed.

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