Kinematics of relative motion of two space bodies in close almost circular orbits

Details Kinematics of relative motion of two space bodies in close almost circular orbits Kinematics of relative motion of two space bodies in close almost circular orbits

Jun 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010cosre..48..260p&link_type=abstract

Cosmic Research, Volume 48, Issue 3, pp.260-264

Physics

Scientific paper

The paper is dedicated to a qualitative investigation of relative motion and close convergences of two space bodies located in close almost circular orbits. This problem is topical due to the asteroid hazard originating from the NEA group asteroids located in the orbits close to that of the Earth. P.E. El’yasberg [1] considered similar problems in the 1960s in relation to Earth’s artificial satellites in close almost circular orbits.

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