On the required accuracy of the theory of motion of perturbing bodies: 2. The inner and general cases / Kuznetsov E.D. // Cosmic Research. - 1998. - V. 36, l. 2. - P. 188-193.

ISSN:

00109525

Type:

Article

Abstract:

The problem of motion of a zero-mass point P in a gravitational field of free mass points is considered. The required accuracy for taking into account the perturbing acceleration of the point P is given. The "inner" (the perturbing body is closer to the attracting center than the perturbed body) and general (arbitrary location of the bodies) cases are considered. The admissible error in representing the motion of perturbing bodies is estimated. The limiting cases are considered. Examples of estimations of the required accuracy of the theory of motion of perturbing bodies are given for Earth's artificial satellites and Solar System bodies. © 1998 MAEe Cyrillic signK Hayκa/Interperiodica Publishing.

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https://www.scopus.com/inward/record.uri?eid=2-s2.0-27144458851&partnerID=40&md5=dcf1e164da780eca4672195ed640fdd5

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Поле	Значение
Link	https://www.scopus.com/inward/record.uri?eid=2-s2.0-27144458851&partnerID=40&md5=dcf1e164da780eca4672195ed640fdd5
Affiliations	Ural State University, ul. Mira 19, Ekaterinburg, 620002, Russian Federation
References	Kuznetsov, E.D., On the Required Accuracy of Theories of Motion of Perturbing Bodies (1994) Astron. Zh., 71 (6), pp. 944-949
Correspondence Address	Kuznetsov, E.D.; Ural State University, ul. Mira 19, Ekaterinburg, 620002, Russian Federation
Language of Original Document	English
Abbreviated Source Title	Cosm. Res.
Source	Scopus