On possible planetary close approaches to high inclination asteroids
The orbital evolution of fictitious high inclination main belt asteroids with movement corresponding to the conditions of the Tisserand invariant for C =C(L1) in the restricted three-body problem has been investigated. The obtained results showed that the bodies with inclinations within 40–80° and 1...
Main Authors: | N. A. Solovaya, E. M. Pittikh |
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Format: | Article |
Language: | English |
Published: |
National Aviation University
2004-12-01
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Series: | Вісник Астрономічної школи |
Online Access: | http://astro.nau.edu.ua/issues/2004_V.5_Iss.1-2/016.html |
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