Published 2007
| Version v1
Book section
Asteroids compositions: Some evidence from Polarimetry
Contributors
Others:
- Service d'aéronomie (SA) ; Université de Versailles Saint-Quentin-en-Yvelines (UVSQ)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
- Institute of Astronomy [Kharkiv] ; V.N. Karazin Kharkiv National University (KhNU)
- Laboratoire Universitaire d'Astrophysique de Nice (LUAN) ; Université Nice Sophia Antipolis (1965 - 2019) (UNS) ; COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-COMUE Université Côte d'Azur (2015-2019) (COMUE UCA)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
- Anil Bhardwaj
Description
Although it cannot provide direct and unambiguous information on the mineralogical composition of an asteroid surface, polarimetry is a very useful tool to get an improved understanding of parameters which are intimately related to surface composition and regolith structure. In recent times there has been a revival in the field of asteroid polarimetry, on the theoretical side, in relation to experimental simulations, and due to the activity of some teams who are engaged in extensive observational campaigns. Some new discoveries of objects exhibiting unprecedented polarimetric properties have been done. The above subjects are briefly reviewed.
Abstract
papier invitéAdditional details
Identifiers
- URL
- https://hal.archives-ouvertes.fr/hal-00196879
- URN
- urn:oai:HAL:hal-00196879v1
Origin repository
- Origin repository
- UNICA