activity
20032026
most citedA low mass for Mars from Jupiter's early gas-driven migration

1.2k citations · 18.3k across the 188 of their papers we have counts for

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Showing 2012Show all

12 papers · 1 filter

astro-ph.EP2012★ 167 cited

Stellar irradiated discs and implications on migration of embedded planets I: equilibrium discs

Bertram Bitsch, Aurélien Crida, Alessandro Morbidelli +2

The strength and direction of migration of low mass planets depends on the disc's thermodynamics. In discs where the viscous heating is balanced by radiative transport, the migrati…

astro-ph.EP2012★ 25 cited

Circum-planetary discs as bottlenecks for gas accretion onto giant planets

Guillaume Rivier, Aurélien Crida, Alessandro Morbidelli +1

With hundreds of exoplanets detected, it is necessary to revisit giant planets accretion models to explain their mass distribution. In particular, formation of sub-jovian planets r…

astro-ph.EP2012★ 17 cited

Dynamical capture in the Pluto-Charon system

P. M. Pires dos Santos, A. Morbidelli, D. Nesvorný

This paper explores the possibility that the progenitors of the small satellites of Pluto got captured in the Pluto-Charon system from the massive heliocentric planetesimal disk in…

astro-ph.EP2012★ 483 cited

Building Terrestrial Planets

Alessandro Morbidelli, Jonathan I. Lunine, David P. O`brien +2

This paper reviews our current understanding of terrestrial planets formation. The focus is on computer simulations of the dynamical aspects of the accretion process. Throughout th…

astro-ph.EP2012★ 234 cited

Dynamics of pebbles in the vicinity of a growing planetary embryo: hydro-dynamical simulations

Alessandro Morbidelli, David Nesvorny

Understanding the growth of the cores of giant planets is a difficult problem. Recently, Lambrechts and Johansen (2012; LJ12) proposed a new model in which the cores grow by the ac…

astro-ph.EP2012★ 113 cited

NOTE: Explaining why the Uranian satellites have equatorial prograde orbits despite the large planetary obliquity

Alessandro Morbidelli, Kleomenis Tsiganis, Konstantin Batygin +2

We show that the existence of prograde equatorial satellites is consistent with a collisional tilting scenario for Uranus. In fact, if the planet was surrounded by a proto-satellit…