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Size-dependent modification of asteroid family Yarkovsky V-shapes
Bryce T. Bolin, Alessandro Morbidelli, Kevin J. Walsh
The thermal properties of the surfaces of asteroids determine the magnitude of the drift rate cause by the Yarkovsky force. In the general case of Main Belt asteroids, the Yarkovsk…
Initial velocity V-shapes of young asteroid families
Bryce T. Bolin, Kevin J. Walsh, Alessandro Morbidelli +1
Ejection velocity fields of asteroid families are largely unconstrained due to the fact that members disperse relatively quickly on Myr time-scales by secular resonances and the Ya…
Is the Grand Tack model compatible with the orbital distribution of main belt asteroids?
Rogerio Deienno, Rodney S. Gomes, Kevin J. Walsh +2
The Asteroid Belt is characterized by the radial mixing of bodies with different physical properties, a very low mass compared to Minimum Mass Solar Nebula expectations and has an…