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(abstract) Spectra of Comet Hale-Bopp

Show simple item record Hanner, M. S. en_US Hayward, T. L. en_US Lynch, D. K. en_US Russell, R. W. en_US 2004-09-30T23:18:49Z 2004-09-30T23:18:49Z 1996-10-23 en_US
dc.identifier.citation Tucson, AZ en_US
dc.identifier.clearanceno 96-1341 en_US
dc.description.abstract The spectra of Hale-Bopp were acquired in mid-1996 at R > 3.5 AU. Strong silicate emission is present in all the spectra. The shape of the feature is very similar to that seen in comet P/Halley. This is the first time that a strong silicate feature has been detected in a comet beyond 2 AU. en_US
dc.format.extent 40399 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other comet silicate Hale-Bopp spectra en_US
dc.title (abstract) Spectra of Comet Hale-Bopp en_US

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