Schwarzschild–Kerr Gravitational Deflection of Potentially Hazardous Space Objects from Their Classical Orbits
- Authors: Yefremov A.P.1
 - 
							Affiliations: 
							
- Institute of Gravitation and Cosmology
 
 - Issue: Vol 24, No 2 (2018)
 - Pages: 113-117
 - Section: Article
 - URL: https://journals.rcsi.science/0202-2893/article/view/176159
 - DOI: https://doi.org/10.1134/S0202289318020159
 - ID: 176159
 
Cite item
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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