We present the first in situ laboratory detection of H2O2 in H+ irradiated
ices at temperatures relevant to the icy Galilean satellites. These experim
ents were motivated by the recent Galileo NIMS detection on Europa of a 3.5
-mu m band identified with H2O2 (R. W. Carlson et al. 1999, Science 283, 20
62-2064). In our laboratory experiments, the IR signature of H2O2 was easil
y observed after irradiation of pure H2O at 16 K, but it was not seen after
irradiation at 80 K. Radiolysis of mixtures of H2O with O-2 or CO2 at 80 K
did produce H2O2 These results show that ices more complex than pure H2O a
re involved in the radiolysis pathway to form H2O2 On Europa. We also repor
t the intrinsic band strength and radiation yield of H2O2 in ice mixtures,
along with possible formation and destruction mechanisms. Sufficient concen
trations of H2O2 can be formed in H2O ices containing O-2 to explain the NI
MS observation. (C) 2000 Academic Press.