The libration points of axisymmetric satellite in the gravitation field of two triaxial rigid bodies

DOI10.1007/BF00113832zbMath0716.70031OpenAlexW2029664938MaRDI QIDQ753525

M. O. Shaker, A. E. El-Dessoky, S. M. El-Shaboury, M. A. El-Tantawy

Publication date: 1991

Published in: Earth, Moon, and Planets (Search for Journal in Brave)

Full work available at URL: https://doi.org/10.1007/bf00113832

zbMATH Keywords

axisymmetric satellite in the gravitation field of two triaxial primariesrestricted problem of three rigid bodies

Mathematics Subject Classification ID

Three-body problems (70F07) Orbital mechanics (70M20)

Related Items (5)

On the stability of the triangular points in the relativistic R3BP with a bigger triaxial primary ⋮ The effect of photogravitational force and oblateness in the perturbed restricted three-body problem ⋮ The effect of oblateness in the perturbed restricted three-body problem ⋮ On the perturbed restricted three-body problem ⋮ Periodic orbits under combined effects of oblateness and radiation in the restricted problem of three bodies

Cites Work

• Sur le probleme des trois corps solides (on the problem of three rigid bodies)
• [https://portal.mardi4nfdi.de/wiki/Publication:3960180 Sur les mouvements r�guliers dans le probl�me des deux corps solides]
• Collinear equilibria and their characteristic exponents in the restricted three-body problem when the primaries are oblate spheroids
• Stationary solutions and their characteristic exponents in the restricted three-body problem when the more massive primary is an oblate spheroid

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