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Orbital determination and dynamics ofresonant extrasolar planetary systems

机译:轨道测定与动态的辐射辐射行星系统

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In this communication we review some properties and applications of mean-motionresonances in extrasolar planetary systems, with particular emphasis on the 2/1 commensura-bility. A first part is devoted to the dynamical structure of the 2/1 resonance, including (but notrestricted to) the so-called apsidal corotations. In a second part we discuss the orbital evolutionof resonant systems under the effects of non-conservative forces. Special attention is given tothe use of apsidal corotations as markers of largescale orbital decay, possibly due to disk-planetinteractions in primordial times. Finally, we analyze the interplay between dynamical analysisand orbital fitting. Using the HD82943 planetary system as an example, we discuss: (i) up towhat point present orbital fits allow us to distinguish between different resonant configurations,and (ii) in what ways may the dynamical structure of resonances be used as a complementarypart of the orbital fitting process.
机译:在这一沟通中,我们审查了额外行星系统中的平均Motientresonances的一些性质和应用,特别强调了2/1个关联效力。第一部分致力于2/1谐振的动态结构,包括(但不当)所谓的暂时的冒险。在第二部分中,我们在非保守力的影响下讨论了谐振系统的轨道进化。特别注意使持续的持续的诊断作为大鼠轨道衰变的标记,可能是由于原始时代的磁盘行星互动。最后,我们分析了动态分析和轨道配件之间的相互作用。使用HD82943行星系统作为示例,我们讨论:(i)向上拖动点目前轨道配合允许我们区分不同的谐振配置,并且(ii)可以在哪些方面可以用作互补的共振结构轨道拟合过程。

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