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Titlebook: Dynamics of Extended Celestial Bodies And Rings; Jean Souchay Book 2006 Springer-Verlag Berlin Heidelberg 2006 Celestial mechanics.Planet.

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發(fā)表于 2025-3-23 12:47:09 | 只看該作者
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發(fā)表于 2025-3-23 14:38:46 | 只看該作者
Facesll body collisions. Such events play a fundamental role in all the stages of the formation and evolution of planetary systems, and more particularly of our Solar System. Laboratory experiments on centimeter-sized targets have been performed to improve our knowledge on this process, but their extrapo
13#
發(fā)表于 2025-3-23 19:35:56 | 只看該作者
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發(fā)表于 2025-3-23 22:35:20 | 只看該作者
Coinsnt this phenomenum thanks to the introduction of two suitable resonant variables. Our model must be considered as a base for future computations; it does not include perturbations due to the in.uence of the other planets, the non-alignment of spin axis with the normal to the equatorial plane and the
15#
發(fā)表于 2025-3-24 05:38:21 | 只看該作者
Chapter 4: Action and the Pragmatic Maximysical processes involving microscopic dust grains, as well as meter-sized boulders. These processes, together with ring composition, can help to understand better the formation and evolution of proto-satellite and proto-planetary disks in the early solar system. The present chapter reviews some fun
16#
發(fā)表于 2025-3-24 08:51:11 | 只看該作者
Jean SouchayIncludes supplementary material:
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發(fā)表于 2025-3-24 12:05:44 | 只看該作者
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發(fā)表于 2025-3-24 15:03:41 | 只看該作者
19#
發(fā)表于 2025-3-24 20:46:17 | 只看該作者
,Physics of the Earth’s Interior, Deformation and Rotation, a fluid core and a solid inner core. Section 2 reviews the concepts that become indispensable when we pass from the model of the Earth as a rigid body to its more realistic model as a deformable planet. In this realistic model, variations in the physical parameters allow us to understand convection
20#
發(fā)表于 2025-3-25 00:59:13 | 只看該作者
Modelling Collisions Between Asteroids: From Laboratory Experiments to Numerical Simulations,ll body collisions. Such events play a fundamental role in all the stages of the formation and evolution of planetary systems, and more particularly of our Solar System. Laboratory experiments on centimeter-sized targets have been performed to improve our knowledge on this process, but their extrapo
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