Water abundance at the surface of C-complex main-belt asteroids

Recently published space-based observations of main-belt asteroids with the AKARI telescope provide a full description of the 3 μm band, related to the presence of OH bearing minerals. Here, we use laboratory spectra of carbonaceous chondrites obtained under controlled atmosphere (CI,CM,CO,CV,CR Tag...

Full description

Bibliographic Details
Main Authors: Beck, Pierre, Eschrig, Jolantha, Potin, Sandra, Prestgard, Trygve, Bonal, Lydie, Quirico, Eric, Schmitt, Bernard
Format: Article in Journal/Newspaper
Language:unknown
Published: arXiv 2020
Subjects:
Online Access:https://dx.doi.org/10.48550/arxiv.2011.00279
https://arxiv.org/abs/2011.00279