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  5. Refining the asteroid taxonomy by polarimetric observations
 

Refining the asteroid taxonomy by polarimetric observations

Journal
ICARUS  
Date Issued
2017
Author(s)
Belskaya, I. N.
•
Fornasier, S.
•
Tozzi, G. P.
•
Gil-Hutton, R.
•
CELLINO, Alberto  
•
Antonyuk, K.
•
Krugly, Yu. N.
•
Dovgopol, A. N.
•
Faggi, S.
DOI
10.1016/j.icarus.2016.11.003
Abstract
We present new results of polarimetric observations of 15 main belt asteroids of different composition. By merging new and published data we determined polarimetric parameters characterizing individual asteroids and mean values of the same parameters characterizing different taxonomic classes. The majority of asteroids show polarimetric phase curves close to the average curve of the corresponding class. We show that using polarimetric data it is possible to refine asteroid taxonomy and derive a polarimetric classification for 283 main belt asteroids. Polarimetric observations of asteroid (21) Lutetia are found to exhibit possible variations of the position angle of the polarization plane over the surface.
Volume
284
Start page
30
Uri
http://hdl.handle.net/20.500.12386/26927
Url
https://www.sciencedirect.com/science/article/abs/pii/S0019103516302032?via%3Dihub
Issn Identifier
0019-1035
Ads BibCode
2017Icar..284...30B
Rights
open.access
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