Late Orbital Instabilities in the Outer Planets Induced by Interaction with a Self-gravitating Planetesimal Disk

We revisit the issue of the cause of the dynamical instability during the so-called Nice model, which describes the early dynamical evolution of the giant planets. In particular, we address the problem of the interaction of planets with a distant planetesimal disk in the time interval between the di...

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Veröffentlicht in:	The Astronomical journal 2011-11, Vol.142 (5), p.152-jQuery1323896812661='48'
Hauptverfasser:	Levison, Harold F, Morbidelli, Alessandro, Tsiganis, Kleomenis, Nesvorný, David, Gomes, Rodney
Format:	Artikel
Sprache:	eng
Schlagworte:	ADIABATIC INVARIANCE ASTROPHYSICS, COSMOLOGY AND ASTRONOMY ENERGY TRANSFER EVOLUTION ICE NEBULAE PLANETS PLUTO PLANET SATELLITES SATURN PLANET SOLAR NEBULA SOLAR SYSTEM EVOLUTION
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