1.2k citations · 18.3k across the 188 of their papers we have counts for
14 papers · 2 filters
A study of 3-dimensional shapes of asteroid families with an application to Eos
Miroslav Brož, Alessandro Morbidelli
In order to fully understand the shapes of asteroids families in the 3-dimensional space of the proper elements it is necessary to compare…
Why do protoplanetary disks appear not massive enough to form the known exoplanet population?
C. F. Manara, A. Morbidelli, T. Guillot
When and how planets form in protoplanetary disks is still a topic of discussion. Exoplanet detection surveys and protoplanetary disk surveys are now providing results that allow u…
Capture into first-order resonances and long-term stability of pairs of equal-mass planets
Gabriele Pichierri, Alessandro Morbidelli, Aurélien Crida
Massive planets form within the lifetime of protoplanetary disks and undergo orbital migration due to planet-disk interactions. When the first planet reaches the inner edge of the…
Dynamical effects on the classical Kuiper Belt during the excited-Neptune model
Rafael Ribeiro de Sousa, Rodney Gomes, Alessandro Morbidelli +1
The link between the dynamical evolution of the giant planets and the Kuiper Belt orbital structure can provide clues and insight about the dynamical history of the Solar System. T…
The excitation of a primordial cold asteroid belt as an outcome of the planetary instability
Rogerio Deienno, Andre Izidoro, Alessandro Morbidelli +3
The main asteroid belt (MB) is low in mass but dynamically excited. Here we propose a new mechanism to excite the MB during the giant planet ('Nice model') instability, which is ex…
Toward a new paradigm for Type II migration
C. M. T Robert, A. Crida, E. Lega +2
Context. Giant planets open gaps in their protoplanetary and subsequently suffer so-called type II migration. Schematically, planets are thought to be tightly locked within their s…