Laboratory UV Photolysis of Planetary Ice Analogs Containing H2O + CO2 (1:1)

Details Laboratory UV Photolysis of Planetary Ice Analogs Containing H2O + CO2 (1:1) Laboratory UV Photolysis of Planetary Ice Analogs Containing H2O + CO2 (1:1)

Mar 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004lpi....35.1450r&link_type=abstract

35th Lunar and Planetary Science Conference, March 15-19, 2004, League City, Texas, abstract no.1450

Computer Science

1

Scientific paper

The composition of icy planetary bodies is affected by photochemical
changes due to UV light. This research is a study of IR spectra of H2O +
CO2 (1:1) mixtures during photolysis. Methods showed efficiencies in
producing near-IR absorptions of photoproducts comparable to planetary
data.

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