Carbonic acid production in H2O : CO2 ices - UV photolysis vs. proton bombardment

Citation
Pa. Gerakines et al., Carbonic acid production in H2O : CO2 ices - UV photolysis vs. proton bombardment, ASTRON ASTR, 357(2), 2000, pp. 793-800
Citations number
31
Categorie Soggetti
Space Sciences
Journal title
ASTRONOMY AND ASTROPHYSICS
ISSN journal
00046361 → ACNP
Volume
357
Issue
2
Year of publication
2000
Pages
793 - 800
Database
ISI
SICI code
0004-6361(200005)357:2<793:CAPIH:>2.0.ZU;2-E
Abstract
We have the unique ability to perform ultraviolet photolysis (similar to 10 eV photon(-1)) and ion irradiation (0.8 MeV p(+)) in the same experimental set-up, with ices created under identical conditions. We present experimen ts that show the formation of carbonic acid (H2CO3) from H2O:CO2 ice mixtur es exposed to either UV photons or high-energy protons. CO and CO3 were als o formed in these experiments. Results show that while H2CO3 is readily for med by p(+) bombardment, its formation by UV photolysis is limited by the p enetration of UV photons into the ice. H2CO3 production pathways are invest igated. Intrinsic IR band strengths are determined for eight IR features of H2CO3. Implications for ices found in various astrophysical environments a re discussed.