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Forventes på lager: 22-05-2017
In an effort to understand the stability of orbits in the solar system, Poincaré applied a Hamiltonian formulation to the equations of planetary motion and studied these differential equations in the limited case of three bodies to arrive at properties of the equations’ solutions, such as orbital resonances and horseshoe orbits.
| Forlag | Springer International Publishing AG |
| Forfatter | Henri Poincare |
| Type | Bog |
| Format | Hardback |
| Sprog | Engelsk |
| Udgave | 1st ed. 2017 |
| Udgivelsesdato | 22-05-2017 |
| Første udgivelsesår | 2017 |
| Serie | Astrophysics and Space Science Library |
| Illustrationer | 9 Illustrations, black and white; XXII, 248 p. 9 illus. |
| Oversætter | Bruce D Popp |
| Originalsprog | Switzerland |
| Sideantal | 248 |
| Indbinding | Hardback |
| Forlag | Springer International Publishing AG |
| Sideoplysninger | 248 pages, 9 Illustrations, black and white; XXII, 248 p. 9 illus. |
| Mål | 160 x 241 x 22 |
| ISBN-13 / EAN-13 | 9783319528984 |