標(biāo)題: Titlebook: Dynamics of Small Solar System Bodies and Exoplanets; Jean J. Souchay,Rudolf Dvorak Book 2010 Springer-Verlag Berlin Heidelberg 2010 Astro [打印本頁] 作者: Clinton 時(shí)間: 2025-3-21 19:39
書目名稱Dynamics of Small Solar System Bodies and Exoplanets影響因子(影響力)
書目名稱Dynamics of Small Solar System Bodies and Exoplanets影響因子(影響力)學(xué)科排名
書目名稱Dynamics of Small Solar System Bodies and Exoplanets網(wǎng)絡(luò)公開度
書目名稱Dynamics of Small Solar System Bodies and Exoplanets網(wǎng)絡(luò)公開度學(xué)科排名
書目名稱Dynamics of Small Solar System Bodies and Exoplanets被引頻次
書目名稱Dynamics of Small Solar System Bodies and Exoplanets被引頻次學(xué)科排名
書目名稱Dynamics of Small Solar System Bodies and Exoplanets年度引用
書目名稱Dynamics of Small Solar System Bodies and Exoplanets年度引用學(xué)科排名
書目名稱Dynamics of Small Solar System Bodies and Exoplanets讀者反饋
書目名稱Dynamics of Small Solar System Bodies and Exoplanets讀者反饋學(xué)科排名
作者: condescend 時(shí)間: 2025-3-21 21:11
The Lyapunov Characteristic Exponents and Their Computation,ped for the computation of the maximal, of few and of all of them. After some historical notes on the first attempts for the numerical evaluation of LCEs, we discuss in detail the multiplicative ergodic theorem of Oseledec [102], which provides the theoretical basis for the computation of the LCEs. 作者: Ischemic-Stroke 時(shí)間: 2025-3-22 00:25 作者: Ingratiate 時(shí)間: 2025-3-22 04:41 作者: Tonometry 時(shí)間: 2025-3-22 12:24 作者: LAVE 時(shí)間: 2025-3-22 14:57 作者: LAVE 時(shí)間: 2025-3-22 20:06
Cometary Dynamics,en different parts of the Solar System. The underlying mechanisms are described with particular emphasis on planetary perturbations. In order to place the dynamical theory into its proper context, we also discuss the distribution of observed cometary orbits and how this is affected by discovery bias作者: 吝嗇性 時(shí)間: 2025-3-23 00:32 作者: 彎曲的人 時(shí)間: 2025-3-23 01:45 作者: 酷熱 時(shí)間: 2025-3-23 09:12
Dynamical Stability of Extra-Solar Planets,xtra-solar planets, we classify the more than 400 planets that have been detected so far according to dynamical aspects. We discuss planetary motion in (i) single-star single-planet, (ii) multi-planet systems, and (iii) binary systems. For the first group we show the application of a general stabili作者: 不能強(qiáng)迫我 時(shí)間: 2025-3-23 12:49 作者: 違反 時(shí)間: 2025-3-23 16:18 作者: Ruptured-Disk 時(shí)間: 2025-3-23 21:41
Lecture Notes in Physicshttp://image.papertrans.cn/e/image/284175.jpg作者: 學(xué)術(shù)討論會(huì) 時(shí)間: 2025-3-23 23:34 作者: Flatus 時(shí)間: 2025-3-24 03:06 作者: 地牢 時(shí)間: 2025-3-24 08:36 作者: 方舟 時(shí)間: 2025-3-24 13:25 作者: 鑒賞家 時(shí)間: 2025-3-24 18:30 作者: Debility 時(shí)間: 2025-3-24 21:41
https://doi.org/10.1007/978-0-85729-422-7od, up to the Magellanic Clouds. Somewhat closer, Gaia will also provide major improvements in the science of asteroids, and more generally to our Solar System, either directly or indirectly. Gaia is a scanning survey telescope aimed to perform high-accuracy astrometry and photometry. More specifica作者: phase-2-enzyme 時(shí)間: 2025-3-25 00:08 作者: Lumbar-Stenosis 時(shí)間: 2025-3-25 05:09
Studying Ctenophora WBR Using ,ance from the Sun (several times 10 000 AU), the comet trajectories are affected by the galactical environment of the Solar System. Two main effects contribute to inject comets from the Oort cloud to the inner Solar system where comets may become observable: the Galactic tide which is due to the dif作者: CAND 時(shí)間: 2025-3-25 09:52 作者: –DOX 時(shí)間: 2025-3-25 15:37
https://doi.org/10.1007/978-1-0716-3553-7xtra-solar planets, we classify the more than 400 planets that have been detected so far according to dynamical aspects. We discuss planetary motion in (i) single-star single-planet, (ii) multi-planet systems, and (iii) binary systems. For the first group we show the application of a general stabili作者: Benzodiazepines 時(shí)間: 2025-3-25 17:47
https://doi.org/10.1007/978-3-642-04458-8Astromety; GAIA; Planet; Solar System; asteroids; cellestial mechanics; comets; dynamical astronomy; exoplan作者: 推測(cè) 時(shí)間: 2025-3-25 21:46 作者: 激勵(lì) 時(shí)間: 2025-3-26 03:13 作者: maculated 時(shí)間: 2025-3-26 07:08 作者: FISC 時(shí)間: 2025-3-26 09:55 作者: avulsion 時(shí)間: 2025-3-26 14:50
https://doi.org/10.1007/978-0-85729-422-7roid observations and the scientific harvest in perspective of what was achieved in the pre-Gaia era. In this lecture we focus on the determination of size of asteroids, shape and rotation, taxonomy, orbits and their improvements with historical highlight and also the dynamical model in general.作者: tangle 時(shí)間: 2025-3-26 19:32
An Introduction to the Dynamics of Trojan Asteroids,l and purely theoretical point of view. In addition, we show how qualitative results can be extracted to describe the properties of Trojan asteroids. We complete our study by summarizing many previous and up-to-date investigations, which focus on their dynamical behavior.作者: crockery 時(shí)間: 2025-3-26 22:59
The Gaia Mission and the Asteroids,roid observations and the scientific harvest in perspective of what was achieved in the pre-Gaia era. In this lecture we focus on the determination of size of asteroids, shape and rotation, taxonomy, orbits and their improvements with historical highlight and also the dynamical model in general.作者: 感情 時(shí)間: 2025-3-27 03:57 作者: 催眠 時(shí)間: 2025-3-27 07:01 作者: Grievance 時(shí)間: 2025-3-27 12:35
https://doi.org/10.1007/978-1-0716-3553-7more complicated from the dynamical point of view—we selected some interesting systems—like Jupiter–Saturn analogs and the close binary systems HD41004 AB, Gliese 86, and γ Cephei—for which we discuss the dynamical stability . Finally, we provide an insight into dynamical contributions to the interdisciplinary research of habitability.作者: filicide 時(shí)間: 2025-3-27 17:30 作者: craving 時(shí)間: 2025-3-27 18:49
The Physics of Asteroids and Their Junction with Dynamics,ting for new physical effects such as Yarkovsky and Yarkovsky–O’Keefe–Radzievskii–Paddack effects. A review of these topic reveals the complexity and the importance of interdisciplinary research on these bodies.作者: Entirety 時(shí)間: 2025-3-28 00:51
Dynamical Stability of Extra-Solar Planets,more complicated from the dynamical point of view—we selected some interesting systems—like Jupiter–Saturn analogs and the close binary systems HD41004 AB, Gliese 86, and γ Cephei—for which we discuss the dynamical stability . Finally, we provide an insight into dynamical contributions to the interdisciplinary research of habitability.作者: 詞匯記憶方法 時(shí)間: 2025-3-28 02:49
Cometary Dynamics,es. We end the review by a preliminary discussion of two current problems dealing with cometary dynamics: the formation and evolution of the scattered disk and the Oort Cloud and the capture of comets into short-period orbits.作者: engrave 時(shí)間: 2025-3-28 07:42 作者: 忘川河 時(shí)間: 2025-3-28 10:36
An Introduction to Common Numerical Integration Codes Used in Dynamical Astronomy,amical astronomy. Six methods are being presented, including a Cash–Karp Runge–Kutta, Radau15, Lie Series, Bulirsch-Stoer, Candy, and a symplectic Hybrid integrator of Mon. Not.R. Astro. Soc. .: 793–799,?]. Their main properties, as for example, the handling of conserved quantities, will be discussed on the basis of the Kepler problem.作者: Minatory 時(shí)間: 2025-3-28 17:00 作者: VOK 時(shí)間: 2025-3-28 19:55
Andrey I. Lavrov,Alexander V. Ereskovskyes. We end the review by a preliminary discussion of two current problems dealing with cometary dynamics: the formation and evolution of the scattered disk and the Oort Cloud and the capture of comets into short-period orbits.作者: deciduous 時(shí)間: 2025-3-29 02:59 作者: MORPH 時(shí)間: 2025-3-29 03:33 作者: COMA 時(shí)間: 2025-3-29 07:43
Book 2010 a thematic school on the topic, held as a result of cooperation between the SYRTE Department of Paris Observatory and the section of astronomy of the Vienna University. Each chapter corresponds to a lecture of several hours given by its author(s). The book therefore represents a necessary and very 作者: 尋找 時(shí)間: 2025-3-29 13:09
