Abstract
The 20,000 years orbital evolution of massless fictitious asteroids located at a border of the Hill’s gravitational sphere has been investigated. The eleven orbits with the eccentricities from 0.0 to 0.4 in five groups of inclinations from 40° to 80° were numerically integrated with planetary perturbations of six major planets, using the numerical integration n-body program with the Everhart’s integrator RA15. For each group time evolution of orbital elements of the asteroids is presented.
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© 1993 Springer Science+Business Media Dordrecht
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Solovaya, N.A., Pittich, E.M. (1993). Evolution of Asteroidal Orbits with High Inclinations. In: Bois, E., Oberti, P., Henrard, J. (eds) Interactions Between Physics and Dynamics of Solar System Bodies. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-1902-3_40
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DOI: https://doi.org/10.1007/978-94-011-1902-3_40
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-4840-8
Online ISBN: 978-94-011-1902-3
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