Methods of Celestial Mechanics: Volume II: Application to Planetary System, Geodynamics and Satellite GeodesySpringer Science & Business Media, 21.11.2005 - 448 Seiten G. Beutler's Methods of Celestial Mechanics is a coherent textbook for students as well as an excellent reference for practitioners. The first volume gives a thorough treatment of celestial mechanics and presents all the necessary mathematical details that a professional would need. The reader will appreciate the well-written chapters on numerical solution techniques for ordinary differential equations, as well as that on orbit determination. In the second volume applications to the rotation of earth and moon, to artificial earth satellites and to the planetary system are presented. The author addresses all aspects that are of importance in high-tech applications, such as the detailed gravitational fields of all planets and the earth, the oblateness of the earth, the radiation pressure and the atmospheric drag. The concluding part of this monumental treatise explains and details state-of-the-art professional and thoroughly-tested software for celestial mechanics. |
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... torques exerted by the respective perturbing bodies); the simulation results are then explained by approximate analytical solutions of the equations of motion. The simulations and the approximate analytic solutions are compared to the ...
... torques exerted by Moon and Sun may be set to zero. • It may be used to study the rotation of the Moon, assuming that the geocentric orbits of Moon and Sun are known. Optionally, the torques exerted by Earth and Sun may be set to zero ...
... torques on Earth and Moon exerted by the planets are very small (due to the geo- and selenocentric distances to the planets and due to the relatively small masses of these bodies) and are neglected here. The rotation of the Earth and ...
... ≈ 242 draconitic. (n and n⊙ are the mean motions of the Moon and the Sun, na is the mean motion of the Moon's perigee) Fig. 2.16. Polar wobble 1981 without torques Fig. 2.18. Euler. 2.2 The Rotation of a Rigid Earth and a Rigid Moon 31.
... torques to zero. One easily sees that the rotation axis is moving on a circle around the figure axis. This behavior will be explained rather easily below. -0.25 -0.2 -0.15 -0.1 -0.05 0 0.05 0.1 0.15 0.2 32 2. The Rotation of Earth and ...
Inhalt
3 | |
6 | |
14 | |
Artificial Earth Satellites | 123 |
Evolution of the Planetary System | 211 |
Variational Equations | 272 |
5 | 301 |
The ComputerPrograms NUMINT and LINEAR | 311 |
The ComputerPrograms SATORB and LEOKIN | 323 |
The ComputerProgram ORBDET 355 | 354 |
The ComputerProgram ERDROT | 371 |
The ComputerProgram PLASYS | 387 |
Elements of Spectral Analysis | 394 |
References | 425 |
Abbreviations and Acronyms 433 | 432 |
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Methods of Celestial Mechanics: Volume II: Application to Planetary System ... Gerhard Beutler Eingeschränkte Leseprobe - 2004 |
Methods of Celestial Mechanics: Volume II: Application to Planetary System ... Gerhard Beutler Keine Leseprobe verfügbar - 2004 |