Mineralogy Of Silicate Dust Particles For Comet 17P/Holmes By Subaru/COMICS

Details Mineralogy Of Silicate Dust Particles For Comet 17P/Holmes By Subaru/COMICS Mineralogy Of Silicate Dust Particles For Comet 17P/Holmes By Subaru/COMICS

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..403y&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.403

Computer Science

Scientific paper

Dust grains and icy materials in comets have been used to investigate the formation conditions of the solar system. It is considered that the existence of crystalline silicate in comets indicates the radial mixing of materials in the early solar nebula. The outburst of comet 17P/Holmes showed on late October, 2007. We carried out low-dispersion spectroscopic observations of 17P/Holmes in midinfrared region with Subaru/COMICS. We show results of our model fitting analysis by using a thermal emission model for this comet. We discuss about the mineral composition for dust grains of 17P/Holmes.

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