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Mid-Infrared Spectra of Comets P/Borrelly, P/Faye, and P/Schaumasse

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dc.contributor.author Hanner, M.S. en_US
dc.contributor.author Lynch, D.K. en_US
dc.contributor.author Russell, R.W. en_US
dc.contributor.author Hackwell, J.A. en_US
dc.contributor.author Kellogg, R. en_US
dc.contributor.author Blaney, D. en_US
dc.date.accessioned 2004-10-04T21:30:43Z
dc.date.available 2004-10-04T21:30:43Z
dc.date.issued 1995 en_US
dc.identifier.citation Icarus en_US
dc.identifier.clearanceno 95-1581 en_US
dc.identifier.uri http://hdl.handle.net/2014/32236
dc.description.abstract A 10 micrometer silicate emission feature has been discovered in the spectra of comets P/Borrelly and P/Faye at R of roughly 1.5 AU although this feature was not observed in P/Schaumasse. A model is presented to show how the shape of the silicate feature can depend on the way in which silicate and absorbing material are mixed in the grains. en_US
dc.format.extent 394107 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other comets dust comets composition comets infrared observations en_US
dc.title Mid-Infrared Spectra of Comets P/Borrelly, P/Faye, and P/Schaumasse en_US


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