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 2015 · astro-ph.EPShow all

14 papers · 2 filters

astro-ph.EP2015★ 220 cited

Fossilized condensation lines in the Solar System protoplanetary disk

A. Morbidelli, B. Bitsch, A. Crida +6

The terrestrial planets and the asteroids dominant in the inner asteroid belt are water poor. However, in the protoplanetary disk the temperature should have decreased below water…

astro-ph.EP2015★ 66 cited

Suppression of type I migration by disk winds

Masahiro Ogihara, Alessandro Morbidelli, Tristan Guillot

Planets less massive than Saturn tend to rapidly migrate inward in protoplanetary disks. This is the so-called type I migration. Simulations attempting to reproduce the observed pr…

astro-ph.EP2015★ 98 cited

Terrestrial Planet Formation Constrained by Mars and the Structure of the Asteroid Belt

André Izidoro, Sean N. Raymond, Alessandro Morbidelli +1

Reproducing the large Earth/Mars mass ratio requires a strong mass depletion in solids within the protoplanetary disk between 1 and 3 AU. The Grand Tack model invokes a specific mi…

astro-ph.EP2015★ 21 cited

Spin-Spin Coupling in the Solar System

Konstantin Batygin, Alessandro Morbidelli

The richness of dynamical behavior exhibited by the rotational states of various solar system objects has driven significant advances in the theoretical understanding of their evol…

astro-ph.EP2015★ 80 cited

Accretion of Uranus and Neptune from inward-migrating planetary embryos blocked by Jupiter and Saturn

Andre Izidoro, Alessandro Morbidelli, Sean N. Raymond +2

Reproducing Uranus and Neptune remains a challenge for simulations of solar system formation. The ice giants' peculiar obliquities suggest that they both suffered giant collisions…

astro-ph.EP2015★ 265 cited

The great dichotomy of the Solar System: small terrestrial embryos and massive giant planet cores

A. Morbidelli, M. Lambrechts, S. Jacobson +1

The basic structure of the solar system is set by the presence of low-mass terrestrial planets in its inner part and giant planets in its outer part. This is the result of the form…