Stationary solutions and their characteristic exponents in the restricted three-body problem when the more massive primary is an oblate spheroid
- 1 March 1976
- journal article
- research article
- Published by Springer Science and Business Media LLC in Celestial Mechanics and Dynamical Astronomy
- Vol. 13 (2), 137-149
- https://doi.org/10.1007/bf01232721
Abstract
No abstract availableKeywords
This publication has 2 references indexed in Scilit:
- Collinear equilibria and their characteristic exponents in the restricted three-body problem when the primaries are oblate spheroidsCelestial Mechanics and Dynamical Astronomy, 1975
- Dynamical Astronomy of the Solar SystemAnnual Review of Astronomy and Astrophysics, 1973