activity
20092024
most citedAccretion and differentiation of the terrestrial planets with implications for the compositions of early-formed Solar System bodies and accretion of water

437 citations · 745 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.IM2024★ 13 cited

The PLATO Mission

Heike Rauer, Conny Aerts, Juan Cabrera +842

PLATO (PLAnetary Transits and Oscillations of stars) is ESA's M3 mission designed to detect and characterise extrasolar planets and perform asteroseismic monitoring of a large numb…

astro-ph.EP2023★ 118 cited

Cold Jupiters and improved masses in 38 Kepler and K2 small planet systems from 3661 HARPS-N radial velocities. No excess of cold Jupiters in small planet systems

A. S. Bonomo, X. Dumusque, A. Massa +31

The exoplanet population characterized by relatively short orbital periods ( d) around solar-type stars is dominated by super-Earths and sub-Neptunes. However, these planets…

astro-ph.EP2014★ 437 cited

Accretion and differentiation of the terrestrial planets with implications for the compositions of early-formed Solar System bodies and accretion of water

David C. Rubie, Seth A. Jacobson, Alessandro Morbidelli +5

In order to test planetary accretion and differentiation scenarios, we integrated a multistage core-mantle differentiation model with N-body accretion simulations. Impacts between…

astro-ph.EP2011★ 31 cited

Considerations on the accretion of Uranus and Neptune by mutual collisions of planetary embryos in the vicinity of Jupiter and Saturn

M. Jakubik, A. Morbidelli, L. Neslusan +1

Modeling the formation of the ice giants Uranus and Neptune is a long-lasting problem in planetary science. Due to gas-drag, collisional damping, and resonant shepherding, the plan…

astro-ph.EP2009★ 146 cited

Constructing the secular architecture of the solar system II: The terrestrial planets

Ramon Brasser, Alessandro Morbidelli, Rodney Gomes +2

We investigate the dynamical evolution of the terrestrial planets during the planetesimal-driven migration of the giant planets. A basic assumption of this work is that giant plane…