Schwarzschild–Kerr Gravitational Deflection of Potentially Hazardous Space Objects from Their Classical Orbits


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Abstract

Distortion of classical elliptical orbits of the Apollo asteroids (crossing the Earth’s orbit) in the gravitational field modeled by the Kerr metric, is calculated, and a numerical assessment is given to the general-relativistic impact on the near-Earth motion of potentially hazardous objects (PHO).

About the authors

A. P. Yefremov

Institute of Gravitation and Cosmology

Author for correspondence.
Email: a.yefremov@rudn.ru
Russian Federation, ul. Miklukho-Maklaya 6, Moscow, 117198


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