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...

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Bibliographic Details
Main Authors: N. A. Solovaya, E. M. Pittikh
Format: Article
Language:English
Published: National Aviation University 2004-12-01
Series:Вісник Астрономічної школи
Online Access:http://astro.nau.edu.ua/issues/2004_V.5_Iss.1-2/016.html

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