Compositional characterisation of the Themis family

Compositional characterisation of the Themis family

Context. It has recently been proposed that the surface composition of icy main-belt asteroids (B-, C-, Cb-, Cg-, P-, and D-types) may be consistent with that of chondritic porous interplanetary dust particles (CP IDPs). Aims. In the light of this new association, we re-examine the surface composit...

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Bibliographic Details
Main Authors: Marsset, M., Vernazza, P., Birlan, M., Dumas, C., Milli, J., Popescu, M., DeMeo, Francesca E, Binzel, Richard P
Other Authors: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Format: Article
Language:en_US
Published: EDP Sciences 2017
Online Access:http://hdl.handle.net/1721.1/106187

Internet

http://hdl.handle.net/1721.1/106187

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