Recent polarimetric observations of comet 67 P/Churyumov-Gerasimenko

dc.contributor.authorAnny-Chantal Levasseur-Regourd1
dc.contributor.authorHadamcik, Edith
dc.contributor.authorSen, A.K.
dc.contributor.authoret.al
dc.date.accessioned2012-08-01T12:20:54Z
dc.date.available2012-08-01T12:20:54Z
dc.date.issued2009-11-24
dc.description.abstractRemote observations of solar light scattered by dust in comet 67P/Churyumov- Gerasimenko coma are of major importance to assess the properties of the dust and thus to prepare the rendezvous of the Rosetta spacecraft with comet 67P/Churyumov-Gerasimenko. We present polarimetric data obtained from India in December 2008 and France in March 2009. Compared with previous observations of this comet and of other Jupiter family comets, they confirm that it is dust-poor, although it may exhibit outbursts leading to the ejection of dust particles from its subsurface, especially after its perihelion passage.en_US
dc.identifier.urihttp://hdl.handle.net/11007/1938
dc.language.isoenen_US
dc.publisherIcy Bodies of the Solar System Proceedings IAU Symposiumen_US
dc.subjectTechniquesen_US
dc.subjectPolarimetricen_US
dc.subjectComets, individual (67P/Churyumov-Gerasimenko)en_US
dc.titleRecent polarimetric observations of comet 67 P/Churyumov-Gerasimenkoen_US
dc.typeArticleen_US

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