The linear stability of libration points of the photogravitational restricted three-body problem when the smaller primary is an oblate spheroid
- 1 January 1987
- journal article
- Published by Springer Science and Business Media LLC in Astrophysics and Space Science
- Vol. 135 (2), 271-281
- https://doi.org/10.1007/bf00641562
Abstract
No abstract availableKeywords
This publication has 8 references indexed in Scilit:
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- Effect of oblateness on triangular solutions at critical massAstrophysics and Space Science, 1979
- On the stability of triangular libration points of the photogravitational restricted circular three-body problemCelestial Mechanics and Dynamical Astronomy, 1978
- Perturbations of the critical mass in the restricted three-body problemAstrophysics and Space Science, 1976
- Stationary solutions and their characteristic exponents in the restricted three-body problem when the more massive primary is an oblate spheroidCelestial Mechanics and Dynamical Astronomy, 1976
- Stability of the points of equilibrium in the restricted problemThe Astronomical Journal, 1967