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Titlebook: Dynamical Trapping and Evolution in the Solar System; Proceedings of the 7 Vassilis V. Markellos,Yoshihide Kozai Conference proceedings 198

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11#
發(fā)表于 2025-3-23 10:33:33 | 只看該作者
Der Borksche Avanciermarsch. (1813)me interval of 2000 years backward and forward is treated. The authors find in all cases that the comet librates temporarily around the 1/1 resonance with Jupiter as a remote jovian satellite during at least two centuries.
12#
發(fā)表于 2025-3-23 15:33:23 | 只看該作者
13#
發(fā)表于 2025-3-23 21:14:04 | 只看該作者
Epilogue, restricted problem of three bodies is used with the Sun and Jupiter as the primaries. Four different cases are studied: direct and retrograde, outside and inside asteroidal orbits. The directions of the asteroidal orbits refer to the synodical reference frame and the positions refer to Jupiter’s or
14#
發(fā)表于 2025-3-24 01:18:15 | 只看該作者
Methode der lichtempfindlichen Zellen,Some mathematical models of the formation of meteor streams are developed. Some of the testable predictions of these models are compared with observations.
15#
發(fā)表于 2025-3-24 04:17:28 | 只看該作者
The Orbital Evolution of the Perseid and Quadrantid Meteor StreamsSome mathematical models of the formation of meteor streams are developed. Some of the testable predictions of these models are compared with observations.
16#
發(fā)表于 2025-3-24 09:09:56 | 只看該作者
https://doi.org/10.1007/978-94-009-7214-8Libration; asteroid; dynamics; earth; galaxies; galaxy; gravitation; gravity; moon; planet; solar system; stabi
17#
發(fā)表于 2025-3-24 12:09:48 | 只看該作者
978-94-009-7216-2D. Reidel Publishing Company, Dordrecht, Holland 1983
18#
發(fā)表于 2025-3-24 18:53:44 | 只看該作者
Dynamical Trapping and Evolution in the Solar System978-94-009-7214-8Series ISSN 0067-0057 Series E-ISSN 2214-7985
19#
發(fā)表于 2025-3-24 20:44:42 | 只看該作者
0067-0057 Overview: 978-94-009-7216-2978-94-009-7214-8Series ISSN 0067-0057 Series E-ISSN 2214-7985
20#
發(fā)表于 2025-3-25 01:40:48 | 只看該作者
Wissenswirtschaft in Deutschland 2002e hypothesis provides a plausible explanation of the origin of the Mimas-Tethys resonance, but it is unsatisfactory for Enceladus-Dione, since their resonance is having little effect on the relative evolution rate of these satellites at present.
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