Icarus, 183, pp. 349-361, http://dx.doi.org./10.1016/j.icarus..03.002
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2006 (v1)Journal articleUploaded on: December 4, 2022
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2006 (v1)Journal article
Icarus, 182, pp. 118-142, http://dx.doi.org./10.1016/j.icarus.2005.12.010
Uploaded on: December 3, 2022 -
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 -
2006 (v1)Journal article
Icarus, 182, pp. 92-117, http://dx.doi.org./10.1016/j.icarus.2005.12.011
Uploaded on: December 3, 2022 -
2022 (v1)Journal article
Context. Asteroid (22) Kalliope is the second largest M-type asteroid in the main belt and is orbited by a satellite, Linus. Whereas the mass of Kalliope is already well constrained thanks to the presence of a moon, its volume is still poorly known, leading to uncertainties on its bulk density and internal structure.Aims. We aim to refine the...
Uploaded on: December 3, 2022