Coorbital Motion about an Oblate Primary

Details Coorbital Motion about an Oblate Primary Coorbital Motion about an Oblate Primary

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009dda....40.1101r&link_type=abstract

American Astronomical Society, DDA meeting #40, #11.01; Bulletin of the American Astronomical Society, Vol. 41, p.904

Astronomy and Astrophysics

Astronomy

Scientific paper

The problem of coorbital motion will be formulated in the Hamiltonian form in case when the primary is oblate. The problem considered will be assumed spatial and not circular. Different forms of the disturbing function will be outlined; the relevant form is developed in terms of Laplace coefficients. The Hamiltonian of the problem will be formed in Dalauny-like canonical elements. The ratio of the primary mass is considered as a small parameter of the first order while the leading oblateness term of the primary is considered of second order.

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