On the problem on resonant rotation of a celestial body in a two-center gravitational field (Q1803472)
From MaRDI portal
 | This is the item page for this Wikibase entity, intended for internal use and editing purposes. Please use this page instead for the normal view: On the problem on resonant rotation of a celestial body in a two-center gravitational field |
scientific article; zbMATH DE number 220913
| Language | Label | Description | Also known as |
|---|---|---|---|
| English | On the problem on resonant rotation of a celestial body in a two-center gravitational field |
scientific article; zbMATH DE number 220913 |
Statements
On the problem on resonant rotation of a celestial body in a two-center gravitational field (English)
0 references
29 June 1993
0 references
The motion of a rigid body \(K\) relatively its centre of mass has been considered. The gravity moments from two attracting centres of masses \(M\) and \(m\) influence the body \(K\). The point mass \(m\) moves on a Kepler's circular orbit in gravitational field of mass \(M\). The motion of the system Venus-Sun-Earth is considered as example.
0 references
rigid body
0 references
Kepler's circular orbit
0 references
Venus-Sun-Earth
0 references
