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Modeling the Gas Flux From a Jupiter-Class Comet Nucleus

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dc.contributor.author Huebner, W. F. en_US
dc.date.accessioned 2004-10-01T21:59:54Z
dc.date.available 2004-10-01T21:59:54Z
dc.date.issued 1995-03 en_US
dc.identifier.citation Toulouse, France en_US
dc.identifier.clearanceno 95-0264 en_US
dc.identifier.uri http://hdl.handle.net/2014/29282
dc.description.abstract Sublimation and gas flux of volatile ices from porous bodies in the Solar System are important, observable phenomena. Surface erosion and dust build-up on a comet nucleus and coma formation are processes attributable to the flux of sublimating gases. Our computer simulations focus on the gas flux from volatile, icy components in the surface layer of a porous, Jupiter-class comet in order to investigate the relationship of the observed relative molecular abundances in the coma with those in then nucleus. We compare results from one-dimensional and two-dimensional models. en_US
dc.format.extent 81965 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Jupiter Comet en_US
dc.title Modeling the Gas Flux From a Jupiter-Class Comet Nucleus en_US


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