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On Non-Stationary Problems of Celestial Mechanics
Published online by Cambridge University Press: 14 August 2015
Extract
Some non-stationary problems of celestial mechanics can be described in an inertial system of right-angled coordinates with gravitational potential of the form:
where is a sufficiently arbitrary function of time and
is the meaning of
in the initial epoch
For example, in a two-body problem of variable mass
we have:
- Type
- Part I: Stability, N- and 3-Body Problems, Variable Mass
- Information
- Symposium - International Astronomical Union , Volume 81: Dynamics of the Solar System , 1979 , pp. 49 - 52
- Copyright
- Copyright © Reidel 1979