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 planet migration occurred after the completion of terrestrial planet formation, such as in the models that link the former to the origin of the Late Heavy Bombardment. The...
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September 7, 2009 (v1)Journal articleUploaded on: December 3, 2022
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May 2018 (v1)Journal article
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Uploaded on: December 4, 2022 -
September 7, 2009 (v1)Journal article
Using numerical simulations, we show that smooth migration of the giant planets through a planetesimal disk leads to an orbital architecture that is inconsistent with the current one: the resulting eccentricities and inclinations of their orbits are too small. The crossing of mutual mean motion resonances by the planets would excite their...
Uploaded on: December 3, 2022 -
December 4, 2007 (v1)Publication
We explore the origin and orbital evolution of the Kuiper belt in the framework of a recent model of the dynamical evolution of the giant planets, sometimes known as the Nice model. This model is characterized by a short, but violent, instability phase, during which the planets were on large eccentricity orbits. One characteristic of this model...
Uploaded on: December 4, 2022 -
July 17, 2007 (v1)Journal article
We study the orbital evolution of the 4 giant planets of our solar system in a gas disk. Our investigation extends the previous works by Masset and Snellgrove (2001) and Morbidelli and Crida (2007, MC07), which focussed on the dynamics of the Jupiter-Saturn system. The only systems that we found to reach a steady state are those in which the...
Uploaded on: February 28, 2023 -
September 8, 2010 (v1)Publication
We use the current orbital structure of large (>50km) asteroids in the main asteroid belt to constrain the evolution of the giant planets when they migrated from their primordial orbits to their current ones. Minton & Malhotra (2009) showed that the orbital distribution of large asteroids in the main belt can be reproduced by an...
Uploaded on: December 4, 2022 -
December 2019 (v1)Journal article
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April 15, 2018 (v1)Conference paper
The main asteroid belt (MB) is low in mass but dynamically excited, with much larger eccentricities and inclinations than the planets. In recent years, the Grand Tack model has been the predominant model capable of reconciling the formation of the terrestrial planets with a depleted but excited MB. Despite this success, the Grand Tack is still...
Uploaded on: December 4, 2022 -
September 1, 2018 (v1)Journal article
International audience
Uploaded on: December 4, 2022 -
March 2020 (v1)Journal article
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Uploaded on: December 3, 2022