| Autor: |
Nakamura, Takeshi, Yoshida, Junzo |
| Zdroj: |
Celestial Mechanics and Dynamical Astronomy; March 1992, Vol. 54 Issue: 1-3 p255-260, 6p |
| Abstrakt: |
The equations of motion of the planar three-body problem split into two parts, called an external part and an internal part. When the third mass approaches zero, the first part tends to the equations of the Kepler motion of the primaries and the second part to the equations of motion of the restricted problem. |
| Databáze: |
Supplemental Index |
| Externí odkaz: |
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