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Identification and yield of carbonic acid and formaldehyde in irradiated icesCarbonic acid, (OH)2CO, was tentatively identified in the IR spectrum of a proton irradiated CO2 + H2O ice mixture. In this report, we present additional evidence for a more definitive identification of (OH)2CO with (1) the infrared spectrum of a residue obtained by proton irradiation of CO2 + D2O ice mixture, and (2) the IR spectra of solid phases of formaldehyde (H2CO), acetone (CH3)2CO, and dimethyl carbonate (OCH3)2CO, which are structurally similar to (OH)2CO. IR characteristics (peak frequencies and complex refractive indices of the compounds in point 2) are also reported. In particular, the integrated absorption coefficients for the C-O band for the compounds in point 2 do not vary by more than 20 percent. Based on these values, we estimate the yields of H2CO and (OH)2CO by proton irradiation or ice mixtures. Both H2CO and (OH)2CO are possible irradiation products of cometary and planetary ices.
Document ID
19930049238
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Dellorusso, Neil
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Khanna, R. K.
(Maryland Univ. College Park, United States)
Moore, M. H.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 16, 2013
Publication Date
March 25, 1993
Publication Information
Publication: Journal of Geophysical Research
Volume: 98
Issue: E3
ISSN: 0148-0227
Subject Category
Lunar And Planetary Exploration
Accession Number
93A33235
Funding Number(s)
CONTRACT_GRANT: NAGW-637
Distribution Limits
Public
Copyright
Other

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