The celestial bodies motion theories: on the required accuracy of the motion theories of the perturbing bodies / Kuznetsov ED // PLANETARY AND SPACE SCIENCE. - 1997. - V. 45, l. 12. - P. 1595-1606.

ISSN/EISSN:

0032-0633 / нет данных

Type:

Article

Abstract:

The equation for calculation of the required accuracy of the perturbing bodies motion theories is obtained. The equation relates the accuracy required to take into account perturbing acceleration, acting on the perturbed body, with the accuracy of the motion theory of the perturbing body. The solutions for estimation of the required accuracy both for the inner and external cases in the spherical coordinates are coincided. The solution for the calculation of the required accuracy for the general case (combining the inner and the external cases) in Cartesian coordinates is obtained. The special cases for the solution in Cartesian are studied. As an example, the estimations of the required accuracy of the motion theories of the solar system planets for some perturbed bodies (the near-Earth asteroid 4179 Toutatis, the main belt asteroid 208 Larcimosa, the trojan asteroid 588 Achilles, the centaur asteroid 5145 Pholus, the Kuiper belt asteroid 1995 QZ9, the comet Halley) are obtained. The conditions of the use of the obtained results are discussed. (C) 1998 Elsevier Science Ltd. All rights reserved.

Author keywords:

нет данных

DOI:

10.1016/S0032-0633(97)00180-3

Web of Science ID:

ISI:000072682600012

Соавторы в МНС:

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Другие поля

Поле	Значение
Month	DEC
Publisher	PERGAMON-ELSEVIER SCIENCE LTD
Address	THE BOULEVARD, LANGFORD LANE, KIDLINGTON, OXFORD OX5 1GB, ENGLAND
Language	English
Research-Areas	Astronomy \& Astrophysics
Web-of-Science-Categories	Astronomy \& Astrophysics
Number-of-Cited-References	3
Journal-ISO	Planet Space Sci.
Doc-Delivery-Number	ZD412