Computer Science
Scientific paper
Oct 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1535p&link_type=abstract
EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1535
Computer Science
Scientific paper
Comet 10P/Tempel 2 (hereafter 10P) was observed after its perihelion passage in 2010 using highdispersion infrared spectroscopy. We present production rates, abundances, and spatial information of eight major volatile species: H2O, HCN, C2H6, CH3OH, NH3, and (3 ) upper limits for NH2, C2H2, and H2CO. In particular, our campaign was contemporaneous with a jet-like feature observed at optical and visual wavelengths in 2010 mid-July. Spatial profiles of primary volatiles display strong enhancements toward the jet direction and to a lesser extent in the anti-jet direction, which favors the idea of direct sublimation in response to local insolation. We discuss possible formation scenarios for this Jupiter Family Comet based on chemical composition and cosmogonic parameters retrieved by our observations.
Bonev Boncho P. .
DiSanti Michael A.
Gibb Erika
Keane Jacqueline V.
Meech Karen Jean
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