Spectral characterisation of 14 V-type candidate asteroids from the MOVIS catalogue
Most of the currently known basaltic (V-type) asteroids are believed to be past or present members of the Vesta dynamical family. The rising discoveries of V-type asteroids that are not linked to the Vesta family dynamically suggest that a number of major basaltic bodies may have been present during the early stages of the solar system. Using the
Matlovič, Pavol et al.
Fecha de publicación:
11
2020