Context. Close encounters with massive asteroids are known to be a mechanism of dynamical mobility that can significantly alter proper elements of minor bodies, and they are the main source of dynamical mobility for medium-sized and large asteroids (D > 20 km, approximately). Aims. Orbital mobility caused by close encounters with (4) Vesta has been studied in the past and could be a viable mechanism to produce the current orbital location of some of the V-type asteroids currently outside the Vesta family. It is well known, however, that the proper frequencies of precession of pericenter g and longitude of the node s of terrestrial planets change when one or more of the other planets is not considered in the integration scheme. For i...
International audienceSmall bodies of the Solar system, like asteroids, trans-Neptunian objects, com...
The known irregular satellites of the giant planets are dormant comet-like objects that reside on st...
Understanding asteroid collisional and dynamical evolution necessitates the use of statistical metho...
Context. Close encounters with massive asteroids are known to be a mechanism of dynamical mobility t...
We numerically estimate the semi-major axis chaotic diffusion of the Vesta family asteroids induced ...
Context.Nearly all members of the Vesta family cross the orbits of (4) Vesta, one of the most massiv...
International audienceThe Vesta family is a known source of near-Earth asteroids (NEAs). Members of ...
Over timescales much longer than an orbital period, the solar system exhibits large-scale chaotic be...
We consider the full Solar System including(1) Ceres and some of the main asteroids, (2) Pallas, (4)...
Context. The orbital instability of minor solar system bodies (asteroids, small satellites, moonlets...
At present, approximately 1500 asteroids are known to evolve inside or sticked to the exterior 1:2 r...
We calculate the eccentricity excitation of asteroids produced by the sweeping ν6 secular resonance ...
Abstract. In the beginning we review briefly the evolution of the ideas on the motion of the bodies ...
The formation of the Hecuba gap close to the 2:1 resonant asteroid mean motion with Jupiter is exami...
Abstract In this paper we present a comprehensive analysis of the dynamics in the region of the (355...
International audienceSmall bodies of the Solar system, like asteroids, trans-Neptunian objects, com...
The known irregular satellites of the giant planets are dormant comet-like objects that reside on st...
Understanding asteroid collisional and dynamical evolution necessitates the use of statistical metho...
Context. Close encounters with massive asteroids are known to be a mechanism of dynamical mobility t...
We numerically estimate the semi-major axis chaotic diffusion of the Vesta family asteroids induced ...
Context.Nearly all members of the Vesta family cross the orbits of (4) Vesta, one of the most massiv...
International audienceThe Vesta family is a known source of near-Earth asteroids (NEAs). Members of ...
Over timescales much longer than an orbital period, the solar system exhibits large-scale chaotic be...
We consider the full Solar System including(1) Ceres and some of the main asteroids, (2) Pallas, (4)...
Context. The orbital instability of minor solar system bodies (asteroids, small satellites, moonlets...
At present, approximately 1500 asteroids are known to evolve inside or sticked to the exterior 1:2 r...
We calculate the eccentricity excitation of asteroids produced by the sweeping ν6 secular resonance ...
Abstract. In the beginning we review briefly the evolution of the ideas on the motion of the bodies ...
The formation of the Hecuba gap close to the 2:1 resonant asteroid mean motion with Jupiter is exami...
Abstract In this paper we present a comprehensive analysis of the dynamics in the region of the (355...
International audienceSmall bodies of the Solar system, like asteroids, trans-Neptunian objects, com...
The known irregular satellites of the giant planets are dormant comet-like objects that reside on st...
Understanding asteroid collisional and dynamical evolution necessitates the use of statistical metho...