Mineralogical and photometric analysis of V-type asteroids

Bibcode
2018EPSC...12.1264M
Medeiros, H.; de Leon, J.; Lazzaro, Daniela; Rondon, Eduardo; Monteiro, Filipe; Popescu, M.; Pinilla-Alonso, Noemi; Arcoverde, Plicida; Morate, D.; Rodrigues, Teresinha; Lorenzi, V.; Landsman, Zoe
Bibliographical reference

European Planetary Science Congress 2018, held 16-21 September 2018 at TU Berlin, Berlin, Germany, id.EPSC2018-1264

Advertised on:
9
2018
Number of authors
12
IAC number of authors
4
Citations
0
Refereed citations
0
Description
Most of the V-types that are known are located in the inner main belt and are members of the Vesta collisional family. The analysis of the photometric and spectroscopic properties of asteroids inside and outside the Vesta family, including V-types in the middle and outer main belt, can answer questions about the existence of differentiated bodies in the asteroid belt and consequently constrain the models of temperature radial extent and variability.
Type
Non-refereed

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