標題: Titlebook: A Comparison of the Dynamical Evolution of Planetary Systems; Proceedings of the S Rudolf Dvorak,Sylvio Ferraz-Mello Conference proceedings [打印本頁] 作者: 粗野的整個 時間: 2025-3-21 16:37
書目名稱A Comparison of the Dynamical Evolution of Planetary Systems影響因子(影響力)
書目名稱A Comparison of the Dynamical Evolution of Planetary Systems影響因子(影響力)學科排名
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書目名稱A Comparison of the Dynamical Evolution of Planetary Systems讀者反饋學科排名
作者: 情感 時間: 2025-3-21 20:56 作者: filicide 時間: 2025-3-22 01:20 作者: 吞吞吐吐 時間: 2025-3-22 07:58 作者: ANTH 時間: 2025-3-22 12:14 作者: 上下連貫 時間: 2025-3-22 15:32
https://doi.org/10.1007/978-3-319-39835-8ss small Trojan-like planets. Several features of the stability regions are also discussed. Finally, the size of the stability region around .. in the elliptic restricted three-body problem is determined as a function of the mass parameter and eccentricity.作者: 小說 時間: 2025-3-22 17:49 作者: 共同生活 時間: 2025-3-22 22:54
Conference proceedings 2005nlinear dynamical systems to the application to real problems. We emphasize the papers on the formation of planetary systems, their stability and also the problem of habitable zones in extrasolar planetary systems. A special topic is the stability of Trojans in our planetary system, where more and m作者: bourgeois 時間: 2025-3-23 01:31
Conference proceedings 2005esults of several numerical experiments unraveled the structure of the stable zone around the librations points. .This volume will be of interest to astronomers and mathematicians interested in Hamiltonian mechanics and in the dynamics of planetary systems.作者: Abrupt 時間: 2025-3-23 07:13
iew, the results of several numerical experiments unraveled the structure of the stable zone around the librations points. .This volume will be of interest to astronomers and mathematicians interested in Hamiltonian mechanics and in the dynamics of planetary systems.978-90-481-7077-7978-1-4020-4466-3作者: probate 時間: 2025-3-23 12:44 作者: Asseverate 時間: 2025-3-23 16:15
G. Cioni,A. Colagrossi,A. Miolaf the basins is found analytically, while the relative area of the basin M. is given by an empirical formula. Further empirical formulae give the exponential decrease of the number of asymptotic orbits that have not yet reached a black hole after . iterations.作者: lambaste 時間: 2025-3-23 18:58
A canonical form guide to symbolic summationrturbation parameter. According to the results obtained, we conclude that the stickiness effect of tori is caused mainly by the hyperbolic invariant sets near the tori, and the diffusion speed becomes larger when orbits diffuse away from the torus.作者: 委屈 時間: 2025-3-23 22:13
F. Parisi-Presicce,A. Pierantonio, a high percentage of ocean area significantly increases the probability for habitability of planets on stable orbits in extrasolar planetary systems. We show that the systems ε Eridani and 55 Cancri are most promising to find dynamic habitable Earth-like planets, while the system ρ Coronae Borealis is most unpromising.作者: 彩色 時間: 2025-3-24 04:34
https://doi.org/10.1007/1-4020-4466-6Astrometry; Celestial mechanics; Galaxy; Planet; Planetary system; Solar System; solar; stellar作者: Hyperalgesia 時間: 2025-3-24 07:15 作者: 入伍儀式 時間: 2025-3-24 13:42
http://image.papertrans.cn/a/image/140300.jpg作者: perpetual 時間: 2025-3-24 16:41 作者: 領帶 時間: 2025-3-24 21:53 作者: 不舒服 時間: 2025-3-25 01:57 作者: 進步 時間: 2025-3-25 06:33
Work, Family, and Their Intersectionimulations of the Trojans in the Sun, Jupiter, Saturn system and on the frequency analysis of these orbits. We give some initial results in the description of the resonant structure that guides the long-term dynamics of this region. Moreover, we are able to connect this global view of the phase spac作者: INERT 時間: 2025-3-25 08:34 作者: 兇殘 時間: 2025-3-25 15:11
https://doi.org/10.1007/978-3-319-39835-8heir osculating Keplerian elements. The method is based on a new resonant Lie-series perturbation theory (Ferraz-Mello, 1997, 2002), which allows the construction of formal solutions in cases where resonant and long-period angles appear simultaneously. For the disturbing function, we used the Beaugé作者: Muffle 時間: 2025-3-25 18:08 作者: ordain 時間: 2025-3-25 23:31 作者: Accord 時間: 2025-3-26 02:13
https://doi.org/10.1007/978-94-011-4603-6onant motion corresponds to periodic motion of the two planets, in a rotating frame, and the position and stability properties of the periodic orbits determine the topology of the phase space and consequently play an important role in the evolution of the system. Several families of symmetric period作者: Alpha-Cells 時間: 2025-3-26 07:35
Albert Prodan,Andrzej Budkowskih smooth center, called SC model. The second model, called CM model, is derived from the SC by inserting a central mass in it, so that all possible differences between the two models are due to the effect of the central mass. The central mass is assumed to be mainly due to a massive central black ho作者: 導師 時間: 2025-3-26 09:17
G. Cioni,A. Colagrossi,A. Miolaits, (b) the asymptotic orbits, with particular emphasis on the homoclinic and heteroclinic orbits, and (c) the basins of attraction of the two black holes. The orbits falling on M. and M. form fractal sets. The asymptotic curves consist of many arcs, separated by gaps. Every gap contains orbits fal作者: fender 時間: 2025-3-26 14:06
S. Antoy,P. Forcheri,J. Gannon,M. T. Molfinoew and useful forms of the virial theorem are obtained for natural Hamiltonian flows of arbitrary dimension. A discrete virial theorem is derived for invariant circles and periodic orbits of natural symplectic maps. A weak and a strong form of the virial theorem are proven for both flows and maps. W作者: Expand 時間: 2025-3-26 18:53
An overview of the TASSO projectiously studied Hamiltonian case (Lega et al., 2003) results agree with the prediction of the Nekhoroshev theorem. Moreover, for values of the perturbation parameter slightly below the critical value of the transition between Nekhoroshev and Chirikov regime we have also found a diffusion of some orbi作者: BOON 時間: 2025-3-26 22:59 作者: BRIBE 時間: 2025-3-27 04:27
G. Cioni,A. Colagrossi,A. Miolaonly on the mass-luminosity relation of the star and climatological and meteorological considerations of Earth-like planets, but neglects atmospheric loss processes due to the interaction with the stellar radiation and particle environment. From the knowledge of the planets in the Solar System, we k作者: Lymphocyte 時間: 2025-3-27 09:16
F. Parisi-Presicce,A. Pierantonioncri, 47 Ursae Majoris, and ρ Coronae Borealis and provide a new tool to assess habitability of extrasolar planetary systems. For determining the habitable zone in these systems an integrated system approach is used taking into account a variety of climatological, biogeochemical, and geodynamical pr作者: 模仿 時間: 2025-3-27 12:13
Local and Global Diffusion Along Resonant Lines in Discrete Quasi-Integrable Dynamical Systems,978-3-540-39600-0作者: 千篇一律 時間: 2025-3-27 14:37 作者: 神刊 時間: 2025-3-27 18:15
A Comparison of the Dynamical Evolution of Planetary Systems978-1-4020-4466-3作者: Gustatory 時間: 2025-3-28 01:52 作者: Needlework 時間: 2025-3-28 04:32
The Stress Process as a Successful Paradigm, for moderate inclinations the size shrinks quite rapidly and disappears completely for . > 60.. Additionally, we found a difference in the dynamics of orbits around .. which — according to the LCE — seem to be more stable than the ones around ...作者: Exterior 時間: 2025-3-28 09:07
https://doi.org/10.1007/978-1-4419-1021-9n of the numbered Trojans follows closely the .. = 1 Gyr level curve, with 86% of the bodies lying inside and 14% outside the stability region. This result is confirmed by a 4.5 Gyr integration of the 246 chaotic numbered Trojans, which showed that 17% of the numbered Trojans are unstable over the a作者: Eructation 時間: 2025-3-28 10:37 作者: SLUMP 時間: 2025-3-28 15:52
Albert Prodan,Andrzej Budkowski regions of phase space, detected by test particles remain empty, i.e. these regions are not occupied by real particles, while many real particles move in unstable regions of phase space describing chaotic orbits. We run self-consistently the two models for more than a Hubble time. During this run, 作者: 親密 時間: 2025-3-28 21:43 作者: caldron 時間: 2025-3-29 02:35
Analytical Proper Elements for the Hilda Asteroids I: Construction of a Formal Solution, to students and researchers in engineering and life sciences, as well as practitioners working with sensing technologies for agricultural monitoring and improvement.?.978-3-030-33489-5978-3-030-33487-1作者: 鬼魂 時間: 2025-3-29 03:09
Chaotic Motions in the Field of Two Fixed Black Holes,r addresses a single emerging technology in depth and describes how manufacturing organizations are adopting the technology. ????The book fills an important niche for manufacturing.? It is a comprehensive, jarg978-3-031-23158-2978-3-031-23156-8作者: Jogging 時間: 2025-3-29 10:05
Front Matterthe recent advances in power system analysis. As the technology advances, continuous study in this area is expected. This chapter summarizes some of the key techniques discussed in the book. The trends of emerging techniques are also given, followed by a list of topics for further reading.作者: Spinous-Process 時間: 2025-3-29 12:51
From Astrometry to Celestial Mechanics: Orbit Determination with Very Short Arcs,ny disciplines. By considering several perspectives we arrive at a composite view that challenges the applicability and effectiveness of purely technological risk analysis (as distinct from organisational risk analysis). This chapter highlights different perspectives that contribute towards an inter作者: 能量守恒 時間: 2025-3-29 16:23 作者: xanthelasma 時間: 2025-3-29 21:06 作者: 聰明 時間: 2025-3-30 03:10
Chaotic Diffusion and Effective Stability of Jupiter Trojans,ually disposed of in landfills or dumped in the sea. The shellfish processing industry is generating about 8.5?million tons of waste every year, with shrimp processing accounting for more than one lakh tonnes of industrial waste. This large amount of waste produced is an appealing opportunity for th作者: 按時間順序 時間: 2025-3-30 06:16 作者: 他日關稅重重 時間: 2025-3-30 11:49 作者: 豪華 時間: 2025-3-30 14:20 作者: 加強防衛(wèi) 時間: 2025-3-30 16:32 作者: 因無茶而冷淡 時間: 2025-3-30 21:07 作者: Paleontology 時間: 2025-3-31 02:34 作者: 實現 時間: 2025-3-31 05:07 作者: Acquired 時間: 2025-3-31 12:04 作者: Oligarchy 時間: 2025-3-31 15:43 作者: Bother 時間: 2025-3-31 20:20
From Astrometry to Celestial Mechanics: Orbit Determination with Very Short Arcs,henomenon across a wide range of disciplines and each disciple brings a particular, distinctive focus. Academic work on risk is often either retrospective, looking at a particular incident, or abstract, considering general properties of the phenomenon. The context of this book is to consider how suc
