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Olivine-rich asteroids in the main asteroid belt
2015Olivine-dominated asteroids, classified as A-types with near-infrared spectral measurements are largely thought to be the mantle remnants of disrupted differentiated small bodies. These A-type asteroids hold clues to asteroid differentiation and to the collisional history of those differentiated bodies.
Demeo, Francesca E. +5 more
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Rogue Asteroids in the Inner Main Asteroid Belt
2014Very red featureless asteroids (spectroscopic D-types) are common among Jupiter Trojans, Hildas, and the outer main belt, and are thought to have formed in the outer solar system. Dynamical models of planetary migration and orbital drift by the Yarkovsky effect predict these D-types could have been transported as close to the sun as the middle main ...
Demeo, Francesca E. +4 more
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Probability for cosmic masses of the main asteroid belt to approach the Earth
Acta Astronautica, 2022Tatiana Salnikova, Alexander Samokhin
exaly
On the Depletion of the Outer Asteroid Belt
1995In the last few years, reasonable success has been achieved in explaining the gaps in semimajor axis distribution of the asteroids. Wisdom (1982, 1983) introduced a mapping technique to study the behavior of bodies at the 3:1 mean motion resonance, which others modified and applied to other gaps (Murray, 1986). They and other researchers (Henrard et al,
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Solar System evolution from compositional mapping of the asteroid belt
Nature, 2014Benoit Carry
exaly