Spins and shapes of basaltic asteroids and the missing mantle problem
Basaltic V-type asteroids are common in the inner part of the Main Asteroid Belt and much less abundant in the mid and outer parts. They are of scientific interest because they sample crusts and mantles of theoretically plentiful differentiated planetesimals that existed in the Solar System four billion years ago. Some Solar System theories suggest
Oszkiewicz, Dagmara et al.
Fecha de publicación:
6
2023