Geodetic Rotation of the Solar System Bodies

Eroshkin, G.; Pashkevich, V.

doi:10.2478/v10018-007-0017-1

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Geodetic Rotation of the Solar System Bodies

Artificial Satellites

Volume 42 (2007): Issue 1 (March 2007)

By: G. Eroshkin and V. Pashkevich

Open Access

|Dec 2007

Abstract

The problem of the geodetic (relativistic) rotation of the major planets, the Moon, and the Sun is studied by using DE404/LE404 ephemeris. For each body the files of the ecliptical components of the vectors of the angular velocity of the geodetic rotation are determined over the time span from AD1000 to AD3000 with one day spacing. The most essential terms of the geodetic rotation are found by means of the least squares method and spectral analysis methods.

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DOI: https://doi.org/10.2478/v10018-007-0017-1 | Journal eISSN: 2083-6104 | Journal ISSN: 1509-3859

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Language: English

Page range: 59 - 70

Published on: Dec 10, 2007

Published by: Polish Academy of Sciences, Space Research Centre

In partnership with: Paradigm Publishing Services

Publication frequency: 4 issues per year

Keywords:

geodetic rotation,

solar system bodies,

ephemeris,

least-squares method,

spectral analysis

Related subjects:

Geosciences,

Geosciences, other

© 2007 G. Eroshkin, V. Pashkevich, published by Polish Academy of Sciences, Space Research Centre
This work is licensed under the Creative Commons License.

Volume 42 (2007): Issue 1 (March 2007)