activity
20172022
most citedDynamical evidence for an early giant planet instability

104 citations · 231 across the 5 of their papers we have counts for

collaborators

9 papers

astro-ph.EP202281 cited

The Exoplanet Radius Valley from Gas-driven Planet Migration and Breaking of Resonant Chains

Andre Izidoro, Hilke E. Schlichting, Andrea Isella +3

The size frequency distribution of exoplanet radii between 1 and 4 is bimodal with peaks at 1.4 and 2.4 , and a valley at 1.8…

astro-ph.EP2021

The effect of a strong pressure bump in the Sun's natal disk: Terrestrial planet formation via planetesimal accretion rather than pebble accretion

André Izidoro, Bertram Bitsch, Rajdeep Dasgupta

Mass-independent isotopic anomalies of carbonaceous and non-carbonaceous meteorites show a clear dichotomy suggesting an efficient separation of the inner and outer solar system. O…

astro-ph.EP202128 cited

Building the Galilean moons system via pebble accretion and migration: A primordial resonant chain

Gustavo Madeira, André Izidoro, Silvia M. Giuliatti Winter

The origins of the Galilean satellites - namely Io, Europa, Ganymede, and Callisto - is not fully understood yet. Here we use N-body numerical simulations to study the formation of…

astro-ph.EP2020

Could Uranus and Neptune form by collisions of planetary embryos?

Alice Chau, Christian Reinhardt, André Izidoro +2

The origin of Uranus and Neptune remains a challenge for planet formation models. A potential explanation is that the planets formed from a population of a few planetary embryos wi…

astro-ph.EP202017 cited

The origins of nearly coplanar, non-resonant systems of close-in super-Earths

Leandro Esteves, André Izidoro, Sean N. Raymond +1

Some systems of close-in "super-Earths" contain five or more planets on non-resonant but compact and nearly coplanar orbits. The Kepler-11 system is an iconic representative of thi…

astro-ph.EP2019104 cited

Dynamical evidence for an early giant planet instability

Rafael Ribeiro de Sousa, Alessandro Morbidelli, Sean N. Raymond +3

The dynamical structure of the Solar System can be explained by a period of orbital instability experienced by the giant planets. While a late instability was originally proposed t…