The surfaces of zero velocity of the restricted three-body problem when the more massive body is luminous, are studied. The properties of the function R which determines these surfaces are given. It is found that the topological properties of the zero velocity surfaces while not affected by the vari
โฆ LIBER โฆ
The geometry of the roche coordinates and zero-velocity curves in the photogravitational three-body problem
โ Scribed by K. E. Papadakis
- Publisher
- Springer Netherlands
- Year
- 1995
- Tongue
- English
- Weight
- 749 KB
- Volume
- 232
- Category
- Article
- ISSN
- 0004-640X
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The stability of the relative equilibrium positions (collinear libration points) of the restricted circular photogravitational threebody problem, in which a passively gravitating point, in addition to experiencing the Newtonian gravity force from the main bodies (stars) also experiences forces of li