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On the required accuracy of the theory of motion of perturbing bodies: 2. The inner and general cases. / Kuznetsov, E. D.
In: Cosmic Research, Vol. 36, No. 2, 1998, p. 188-193.

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@article{eb764e2553bd4d64b94d0db6eedde174,
title = "On the required accuracy of the theory of motion of perturbing bodies: 2. The inner and general cases",
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. {\textcopyright} 1998 MAEe Cyrillic signK Hayκa/Interperiodica Publishing.",
author = "Kuznetsov, {E. D.}",
year = "1998",
language = "English",
volume = "36",
pages = "188--193",
journal = "Cosmic Research",
issn = "0010-9525",
publisher = "Pleiades Publishing",
number = "2",

}

RIS

TY - JOUR

T1 - On the required accuracy of the theory of motion of perturbing bodies: 2. The inner and general cases

AU - Kuznetsov, E. D.

PY - 1998

Y1 - 1998

N2 - 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.

AB - 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.

UR - http://www.scopus.com/inward/record.url?partnerID=8YFLogxK&scp=27144458851

M3 - Article

VL - 36

SP - 188

EP - 193

JO - Cosmic Research

JF - Cosmic Research

SN - 0010-9525

IS - 2

ER -

ID: 54649791