The Moon's influence on the location of the Sun-Earth exterior libration point
β Scribed by Robert W. Farquhar
- Publisher
- Springer Netherlands
- Year
- 1970
- Tongue
- English
- Weight
- 114 KB
- Volume
- 2
- Category
- Article
- ISSN
- 1572-9478
No coin nor oath required. For personal study only.
π SIMILAR VOLUMES
The translational-rotational motion of an orbital station in the Earth-Moon system is investigated. The orbital station is regarded as a body of variable composition with a solid shell and a low-thrust jet engine placed on it, having constant autonomous orientation in a system of coordinates rotatin
Consider the Earth-Moon-particle system as a Restricted Three Body Problem. There are two equilateral libration points. In the actual world system, those points are no longer relative equilibrium points mainly due to the effect of the Sun and to the noncircular motion of the Moon around the Earth. I