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: | , |
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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 |