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Olivine-rich asteroids in the main asteroid belt

2015
Olivine-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
openaire   +1 more source

Formation of Main Belt Asteroids

2022
Hubert Klahr   +2 more
openaire   +1 more source

Main-Belt Asteroids

2014
Daniel T. Britt   +2 more
openaire   +1 more source

Late accretion of Ceres-like asteroids and their implantation into the outer main belt

Nature Astronomy, 2023
Sean Raymond   +2 more
exaly  

Fine-regolith production on asteroids controlled by rock porosity

Nature, 2021
Saverio Cambioni   +2 more
exaly  

Main-Belt Asteroids

2007
Britt, Daniel T.   +2 more
openaire   +2 more sources

On the spatial distribution of main belt asteroids

2014
We investigate here the distribution of main belt asteroids in the space with respect to the ecliptic-equinox J2000. We identify and confirm a sinusoidal behaviour of this distribution, which disappears when the inclination is given with respect to Jupiter's orbital plane, or with respect to the invariable plane (IP).
Souami, Damya   +2 more
openaire   +1 more source

Photometric Geodesy of main-belt asteroids

Icarus, 1987
S.B. Weideenschilling   +5 more
openaire   +1 more source

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