STABILITY OF THE KEPLER-11 SYSTEM AND ITS ORIGIN

A significant fraction of Kepler systems are closely packed, largely coplanar, and circular. We study the stability of a six-planet system, Kepler-11, to gain insights on the dynamics and formation history of such systems. Using a technique called "frequency maps" as fast indicators of lon...

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Veröffentlicht in:	The Astrophysical journal 2014-11, Vol.795 (1), p.1-8
Hauptverfasser:	Mahajan, Nikhil, Wu, Yanqin
Format:	Artikel
Sprache:	eng
Schlagworte:	ASTROPHYSICS, COSMOLOGY AND ASTRONOMY CHAOS THEORY Dynamical systems Dynamics Eccentricity EVOLUTION EXCITATION GAIN INSTABILITY MASS TRANSFER MIGRATION Orbitals Origins PLANETS SATELLITES SPACE STABILITY STARS STELLAR WINDS TRAPPING TWO-BODY PROBLEM
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