| タイトル | Torques on a nearly rigid body in a relativistic gravitational field |
| 本文（外部サイト） | http://hdl.handle.net/2060/19800022784 |
| 著者（英） | Caporali, A. |
| 著者所属（英） | NASA Marshall Space Flight Center |
| 発行日 | 1980-08-01 |
| 言語 | eng |
| 内容記述 | The effect of post-Newtonian potentials on the rotation of a nearly rigid body is shown to consist of a precession and a torque. The frequency of the precession can be exactly represented by means of suitable differential operators. The relativistic torques in the quadrupole approximation depend on the instantaneous orientation of the principal axes of one body with respect to the position like the classical torque and velocity of the other. For a relatively low mass body, such as a gyroscope, these velocity-dependent torques have no observable consequences. |
| NASA分類 | ASTROPHYSICS |
| レポートNO | 80N31289
NASA-TM-78295 |
| 権利 | No Copyright |
| URI | https://repository.exst.jaxa.jp/dspace/handle/a-is/171430 |
