Comparison of the Organic Composition of Cometary Samples with Residues Formed from the UV Irradiation of Astrophysical Ice Analogs

Details Comparison of the Organic Composition of Cometary Samples with Residues Formed from the UV Irradiation of Astrophysical Ice Analogs Comparison of the Organic Composition of Cometary Samples with Residues Formed from the UV Irradiation of Astrophysical Ice Analogs

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.2078m&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.2078

Astronomy and Astrophysics

Astrophysics

Scientific paper

We present C-, N-, and O-XANES results of organic residues produced in
the laboratory from the UV irradiation of astrophysical ice analogs
containing H2O, CO, CH3OH, NH3, in order to mimic processes that may
occur in comets.

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