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(Reference retrieved automatically from Web of Science through information on FAPESP grant and its corresponding number as mentioned in the publication by the authors.)

Nonsphericity of the Moon and Near Sun-Synchronous Polar Lunar Orbits

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Author(s):
dos Santos Carvalho, Jean Paulo [1] ; de Moraes, Rodolpho Vilhena [1] ; Bertachini de Almeida Prado, Antonio Fernando [2]
Total Authors: 3
Affiliation:
[1] Univ Estadual Paulista, BR-12516410 Guaratingueta, SP - Brazil
[2] INPE, Div Space Mech & Control, BR-12227010 Sao Jose Dos Campos, SP - Brazil
Total Affiliations: 2
Document type: Journal article
Source: MATHEMATICAL PROBLEMS IN ENGINEERING; 2009.
Web of Science Citations: 6
Abstract

Herein, we consider the problem of a lunar artificial satellite perturbed by the nonuniform distribution of mass of the Moon taking into account the oblateness (J(2)) and the equatorial ellipticity (sectorial term C(22)). Using Lie-Hori method up to the second order short-period terms of the Hamiltonian are eliminated. A study is done for the critical inclination in first and second order of the disturbing potential. Coupling terms due to the nonuniform distribution of mass of the Moon are analyzed. Numerical simulations are presented with the disturbing potential of first and second order is. It an approach for the behavior of the longitude of the ascending node of a near Sun-synchronous polar lunar orbit is presented. Copyright (C) 2009 Jean Paulo dos Santos Carvalho et al. (AU)

FAPESP's process: 06/04997-6 - Close approach problems in orbital dynamics
Grantee:Rodolpho Vilhena de Moraes
Support type: Research Projects - Thematic Grants