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.