Astronomy and Astrophysics – Astronomy
Scientific paper
Dec 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984azh....61.1205a&link_type=abstract
(Astronomicheskii Zhurnal, vol. 61, Nov.-Dec. 1984, p. 1205-1210) Soviet Astronomy (ISSN 0038-5301), vol. 28, Nov.-Dec. 1984, p.
Astronomy and Astrophysics
Astronomy
Asteroids, Celestial Mechanics, Orbit Perturbation, Secular Variations, Solar Orbits, Three Body Problem, Approximation, Gas Giant Planets, Jupiter (Planet), Orbit Calculation, Planetary Orbits, Planetary Rings
Scientific paper
The internal variant of the generalized problem of three fixed centers is applied to determine an intermediate orbit for the asteroid 126 Vellade, extending the method of Arazov and Gabibov (1979) to account, in a first approximation, for the secular perturbations of all the outer planets. The results are presented in tables and compared with those obtained by numerical integration and with observations over a 75-yr period. It is shown that intermediate orbits determined by the present method for nonresonant asteroids with a between 2.15 and 4.26 are more useful starting points for dynamic investigations than the corresponding Keplerian intermediate orbits.
Arazov G. T.
Gabibov S. A.
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