Journal of Nonlinear Mathematical Physics

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Volume 8, Issue Supplement, February 2001, Pages 289 - 293

A Dynamical System: Mars and its Satellite

Authors
Piotr Wąż
Corresponding Author
Piotr Wąż
Available Online 1 February 2001.
DOI
10.2991/jnmp.2001.8.s.50How to use a DOI?
Abstract

A description of the most accurate analytical theory of the motion of Phobos, so far constructed, is presented. Several elements of the gravitational field of Mars, gravitational interactions between Phobos and Mars, Deimos and Jupiter, as well as tidal effects due to the interaction between the Sun and Mars, never considered before, have been taken into account. The theory is based on the model of two fixed gravitational centers.

Copyright
© 2006, the Authors. Published by Atlantis Press.
Open Access
This is an open access article distributed under the CC BY-NC license (http://creativecommons.org/licenses/by-nc/4.0/).

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<Previous Article In Issue
Next Article In Issue>
Journal
Journal of Nonlinear Mathematical Physics
Volume-Issue
8 - Supplement
Pages
289 - 293
Publication Date
2001/02/01
ISBN
91-631-0262-5
ISSN (Online)
1776-0852
ISSN (Print)
1402-9251
DOI
10.2991/jnmp.2001.8.s.50How to use a DOI?
Copyright
© 2006, the Authors. Published by Atlantis Press.
Open Access
This is an open access article distributed under the CC BY-NC license (http://creativecommons.org/licenses/by-nc/4.0/).

Cite this article

risenwbib
TY  - JOUR
AU  - Piotr Wąż
PY  - 2001
DA  - 2001/02/01
TI  - A Dynamical System: Mars and its Satellite
JO  - Journal of Nonlinear Mathematical Physics
SP  - 289
EP  - 293
VL  - 8
IS  - Supplement
SN  - 1776-0852
UR  - https://doi.org/10.2991/jnmp.2001.8.s.50
DO  - 10.2991/jnmp.2001.8.s.50
ID  - Wąż2001
ER  -