Many asteroid families are identified and well characterized all over the main asteroid belt. Interestingly, however, none of them are older than 4 Gyr. Many mechanisms have been proposed to disperse such old primordial asteroid families that presumably have existed, but only very few have really worked. Here we present a plausible mechanism...
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March 1, 2016 (v1)Journal articleUploaded on: December 4, 2022
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2005 (v1)Journal article
The 2/1 mean motion resonance with Jupiter, intersecting the main asteroid belt at ≈3.27 au, contains a small population of objects. Numerical investigations have classified three groups within this population: asteroids residing on stable orbits (i.e. Zhongguos), those on marginally stable orbits with dynamical lifetimes of the order of 100...
Uploaded on: December 4, 2022 -
August 11, 2013 (v1)Journal article
International audience
Uploaded on: December 4, 2022