派博傳思國際中心

標(biāo)題: Titlebook: Dynamical Trapping and Evolution in the Solar System; Proceedings of the 7 Vassilis V. Markellos,Yoshihide Kozai Conference proceedings 198 [打印本頁]

作者: CAP    時(shí)間: 2025-3-21 19:57
書目名稱Dynamical Trapping and Evolution in the Solar System影響因子(影響力)




書目名稱Dynamical Trapping and Evolution in the Solar System影響因子(影響力)學(xué)科排名




書目名稱Dynamical Trapping and Evolution in the Solar System網(wǎng)絡(luò)公開度




書目名稱Dynamical Trapping and Evolution in the Solar System網(wǎng)絡(luò)公開度學(xué)科排名




書目名稱Dynamical Trapping and Evolution in the Solar System被引頻次




書目名稱Dynamical Trapping and Evolution in the Solar System被引頻次學(xué)科排名




書目名稱Dynamical Trapping and Evolution in the Solar System年度引用




書目名稱Dynamical Trapping and Evolution in the Solar System年度引用學(xué)科排名




書目名稱Dynamical Trapping and Evolution in the Solar System讀者反饋




書目名稱Dynamical Trapping and Evolution in the Solar System讀者反饋學(xué)科排名





作者: Mawkish    時(shí)間: 2025-3-21 22:13
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.
作者: 匯總    時(shí)間: 2025-3-22 01:13
Wissenskommunismus und Wissenskapitalismusy problem are given. This problem was analyzed in part by Kane and Marsh (1971), Markeev (1967a,b). However the present investigation is formulated in terms of hamiltonian mechanics. The final results will by used to study nonlinear effects connected with the gravitational influence of the “second”
作者: MULTI    時(shí)間: 2025-3-22 08:21

作者: Hearten    時(shí)間: 2025-3-22 12:12

作者: precede    時(shí)間: 2025-3-22 13:36

作者: precede    時(shí)間: 2025-3-22 18:51

作者: 誘惑    時(shí)間: 2025-3-22 23:49
,Das Rechnen bei den Griechen und R?mern,obertson effect. New particles can also be generated in a stream through being released from the nucleus of a comet. We summarise the main physical effects, discuss models for meteor stream evolution and give a brief account of the observational data available.
作者: constitute    時(shí)間: 2025-3-23 02:41

作者: deciduous    時(shí)間: 2025-3-23 06:07

作者: 非秘密    時(shí)間: 2025-3-23 10:33
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.
作者: REIGN    時(shí)間: 2025-3-23 15:33

作者: 直言不諱    時(shí)間: 2025-3-23 21:14
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
作者: 時(shí)代    時(shí)間: 2025-3-24 01:18
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.
作者: GLIDE    時(shí)間: 2025-3-24 04:17
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.
作者: apropos    時(shí)間: 2025-3-24 09:09
https://doi.org/10.1007/978-94-009-7214-8Libration; asteroid; dynamics; earth; galaxies; galaxy; gravitation; gravity; moon; planet; solar system; stabi
作者: nitric-oxide    時(shí)間: 2025-3-24 12:09
978-94-009-7216-2D. Reidel Publishing Company, Dordrecht, Holland 1983
作者: Budget    時(shí)間: 2025-3-24 18:53
Dynamical Trapping and Evolution in the Solar System978-94-009-7214-8Series ISSN 0067-0057 Series E-ISSN 2214-7985
作者: 殺死    時(shí)間: 2025-3-24 20:44
0067-0057 Overview: 978-94-009-7216-2978-94-009-7214-8Series ISSN 0067-0057 Series E-ISSN 2214-7985
作者: 貪婪性    時(shí)間: 2025-3-25 01:40
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.
作者: 諷刺滑稽戲劇    時(shí)間: 2025-3-25 04:22

作者: Daily-Value    時(shí)間: 2025-3-25 10:14
Wissenswirtschaft in Deutschland 2002ng a new regularizing function..We make an application to the zonal earth satellite, considering the hamiltonian function through the harmonic J.. After the angular variable u has been removed, we introduce a new time and we reduce the problem to a linear equation.
作者: arbovirus    時(shí)間: 2025-3-25 14:47
Der Raum,rmulae are derived. And then, orbital evolutions of the nine major planets in solar system during about 2,100,000 years are investigated numerically. The method applied here is in principle suitable for the orbits of arbitrary eccentricities and inclinations.
作者: 蘑菇    時(shí)間: 2025-3-25 19:42
,Das Rechnen bei den Griechen und R?mern,obertson effect. New particles can also be generated in a stream through being released from the nucleus of a comet. We summarise the main physical effects, discuss models for meteor stream evolution and give a brief account of the observational data available.
作者: insightful    時(shí)間: 2025-3-25 21:16

作者: 無孔    時(shí)間: 2025-3-26 00:13

作者: Esophagus    時(shí)間: 2025-3-26 05:29

作者: 大洪水    時(shí)間: 2025-3-26 10:04
A Re-Consideration of the Evolution Hypothesis of the Origin of the Resonances Among Saturn’s Satelle 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.
作者: genuine    時(shí)間: 2025-3-26 16:02
Orientation of a Satellite Located at the Libration Point in the Restricted Three-Body Problemy problem are given. This problem was analyzed in part by Kane and Marsh (1971), Markeev (1967a,b). However the present investigation is formulated in terms of hamiltonian mechanics. The final results will by used to study nonlinear effects connected with the gravitational influence of the “second” central body.
作者: Alpha-Cells    時(shí)間: 2025-3-26 19:16

作者: 改進(jìn)    時(shí)間: 2025-3-26 22:38

作者: Fortify    時(shí)間: 2025-3-27 03:38

作者: 歪曲道理    時(shí)間: 2025-3-27 05:35

作者: Cupping    時(shí)間: 2025-3-27 11:02
Families of Asteroidsral aspects. It seems to the author that there are two kinds of the families, one being very compact in the phase space and containing many faint as well as a few bright asteroids and one being rather loose and bounded by secular and mean motion commensurable regions.
作者: cacophony    時(shí)間: 2025-3-27 16:25

作者: 雄辯    時(shí)間: 2025-3-27 21:24

作者: Harridan    時(shí)間: 2025-3-27 22:23

作者: Excitotoxin    時(shí)間: 2025-3-28 03:17

作者: 匍匐    時(shí)間: 2025-3-28 09:50

作者: aerobic    時(shí)間: 2025-3-28 13:31
Epilogue,ability of asteroids, the results being also applicable to comets and meteor streams. The evolution of the solar system may be studied using planets, satellites or smaller bodies like asteroids. The unquestionable advantage of approaching the problem via the investigation of asteroids is that there
作者: 善變    時(shí)間: 2025-3-28 16:13
Zur Wissensunordnung des Internetsral case can be derived from a Hamiltonian solution by a method of variation of constants. The crossing of a libration region causes a retardation in the increase of the semi-major axis. These results are confirmed by numerical integration and orders of magnitude of this retardation are given.
作者: 使?jié)M足    時(shí)間: 2025-3-28 21:49
High Order Resonances in the Evolution of the Lunar Orbitral case can be derived from a Hamiltonian solution by a method of variation of constants. The crossing of a libration region causes a retardation in the increase of the semi-major axis. These results are confirmed by numerical integration and orders of magnitude of this retardation are given.
作者: Pde5-Inhibitors    時(shí)間: 2025-3-29 00:41
Theory of the Libration of the Moonhe Moon is assumed to be rigid and its orbital motion is described by the ELP 2000 solution (Chapront and Chapront-Touzé 1981) for the main problem of lunar theory with planetary perturbations and influence of the non-sphericity of the Earth. Comparisons with other theories (Migus 1980 and Eckhardt 1981) are also presented.
作者: 負(fù)擔(dān)    時(shí)間: 2025-3-29 06:54

作者: Enthralling    時(shí)間: 2025-3-29 08:31

作者: inculpate    時(shí)間: 2025-3-29 14:32

作者: 指派    時(shí)間: 2025-3-29 15:43

作者: rectum    時(shí)間: 2025-3-29 20:52
Marsch des Bataillons Garde. (1806) distance of 0.015 AU, in 1770, and was discovered. The final, very close encounter with Jupiter, in 1779, removed the comet from observability, sending it into an orbit of perihelion distance in excess of 5 AU (Kazimirchak-Polonskaya, 1967).
作者: Mechanics    時(shí)間: 2025-3-30 03:32

作者: 故意    時(shí)間: 2025-3-30 06:17

作者: forebear    時(shí)間: 2025-3-30 11:04
Orientation of a Satellite Located at the Libration Point in the Restricted Three-Body Problemy problem are given. This problem was analyzed in part by Kane and Marsh (1971), Markeev (1967a,b). However the present investigation is formulated in terms of hamiltonian mechanics. The final results will by used to study nonlinear effects connected with the gravitational influence of the “second”
作者: OGLE    時(shí)間: 2025-3-30 15:45
Theory of the Libration of the Moonld. This field is represented through its fourth degree harmonics for the torque due to the Earth (the second degree for the torque due to the Sun). The Moon is assumed to be rigid and its orbital motion is described by the ELP 2000 solution (Chapront and Chapront-Touzé 1981) for the main problem of
作者: 擴(kuò)大    時(shí)間: 2025-3-30 20:28

作者: Formidable    時(shí)間: 2025-3-30 21:30

作者: 傳授知識    時(shí)間: 2025-3-31 03:53





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