Three characteristic orbital parameters for the Trojan group of asteroids

Details Three characteristic orbital parameters for the Trojan group of asteroids Three characteristic orbital parameters for the Trojan group of asteroids

Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987a%26a...175..292b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 175, no. 1-2, March 1987, p. 292-298.

Astronomy and Astrophysics

Astronomy

26

Asteroids, Gravitational Effects, Librational Motion, Orbital Elements, Trojan Orbits, Dynamic Models, Eccentricity, Inclination, Jupiter (Planet), Numerical Integration, Saturn (Planet), Asteroids, Trojan Asteroids, Characteristics, Orbits, Parameters, Models, Astronomy, Procedure, Techique, Amplitude, Libration, Eccentricity, Inclination, Catalog, Data

Scientific paper

The three 'proper element' orbital parameters derivable for the Trojan asteroids by the procedure presented characterize the amplitude of libration, the proper eccentricity, and the proper inclination. While the results obtained are primarily based on numerical integrations encompassing the behavior of Jupiter and Saturn over + or - 73,000 years, it is anticipated that the three proper elements are constant over a much longer time interval. The results are presented in tabular form.

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