Aims. We locate escape routes from the main asteroid belt, particularly into the near-Earth-object (NEO) region, and estimate the relative fluxes for different escape routes as a function of object size under the influence of the Yarkovsky semimajor-axis drift. Methods. We integrated the orbits of 78 355 known and 14 094 cloned main-belt objects and Cybele and Hilda asteroids (hereafter collectively called MBOs) for 100 Myr and recorded the characteristics of the escaping objects. The selected sample of MBOs with perihelion distance q > 1.3 au and semimajor axis a < 4.1 au is essentially complete, with an absolute magnitude limit ranging from HV < 15.9 in the inner belt (a < 2.5 au) to HV < 14.4 in the outer belt (2.5 au < a < 4.1 a...
The Yarkovsky effect is a thermal process acting upon the orbits of small celestial bodies, which ca...
International audienceThe Vesta family is a known source of near-Earth asteroids (NEAs). Members of ...
Aims. Ceres and Vesta are the two largest bodies in the main asteroid belt (MB) and have been extens...
We have identified and quantified semimajor axis drifts in near-Earth asteroids (NEAs) by performing...
We have identified and quantified semimajor axis drifts in near-Earth asteroids (NEAs) by performing...
The size distribution of main-belt of asteroids is determined primarily by collisional processes. La...
We investigate the relevance of the Yarkovsky effect for the origin of kilometer and multikilometer ...
Context. The Yarkovsky effect is a weak non-gravitational force leading to a small variation of the ...
Near-Earth Objects (NEOs) are a transient population of small bodies with orbits near or in the terr...
Aims. We developed a six-part collisional evolution model of the main asteroid belt (MB) and used it...
International audienceContext. The Yarkovsky effect is a weak non-gravitational force leading to a s...
We investigate the flux of main-belt asteroid fragments into resonant orbits converting them into ne...
Asteroid (101955) Bennu, the target of NASA\u27s OSIRIS-REx sample return mission, is a D approximat...
Context. It is widely accepted that the current distribution of material in the main asteroidal belt...
Finally, the Yarkovsky semimajor axis drift may be important in transporting to the main resonances ...
The Yarkovsky effect is a thermal process acting upon the orbits of small celestial bodies, which ca...
International audienceThe Vesta family is a known source of near-Earth asteroids (NEAs). Members of ...
Aims. Ceres and Vesta are the two largest bodies in the main asteroid belt (MB) and have been extens...
We have identified and quantified semimajor axis drifts in near-Earth asteroids (NEAs) by performing...
We have identified and quantified semimajor axis drifts in near-Earth asteroids (NEAs) by performing...
The size distribution of main-belt of asteroids is determined primarily by collisional processes. La...
We investigate the relevance of the Yarkovsky effect for the origin of kilometer and multikilometer ...
Context. The Yarkovsky effect is a weak non-gravitational force leading to a small variation of the ...
Near-Earth Objects (NEOs) are a transient population of small bodies with orbits near or in the terr...
Aims. We developed a six-part collisional evolution model of the main asteroid belt (MB) and used it...
International audienceContext. The Yarkovsky effect is a weak non-gravitational force leading to a s...
We investigate the flux of main-belt asteroid fragments into resonant orbits converting them into ne...
Asteroid (101955) Bennu, the target of NASA\u27s OSIRIS-REx sample return mission, is a D approximat...
Context. It is widely accepted that the current distribution of material in the main asteroidal belt...
Finally, the Yarkovsky semimajor axis drift may be important in transporting to the main resonances ...
The Yarkovsky effect is a thermal process acting upon the orbits of small celestial bodies, which ca...
International audienceThe Vesta family is a known source of near-Earth asteroids (NEAs). Members of ...
Aims. Ceres and Vesta are the two largest bodies in the main asteroid belt (MB) and have been extens...