On analysis of close encounters of two cosmic bodies in near almost-circular orbits

Details On analysis of close encounters of two cosmic bodies in near almost-circular orbits On analysis of close encounters of two cosmic bodies in near almost-circular orbits

Dec 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010cosre..48..526p&link_type=abstract

Cosmic Research, Volume 48, Issue 6, pp.526-533

Physics

Scientific paper

This paper is devoted to the study of relative motion and close encounters of two cosmic bodies located in near almost-circular orbits. This problem is topical due to the asteroid hazard proceeding from the NEA group asteroids located in the near-Earth orbits. The (99942) Apophis asteroid, a representative of this group discovered in July 2004 by the Kitt Peak observatory (Arizona), is considered as an example.

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