14:15 〜 14:30
[PPS09-03] パラH2Oの凝集によって生成した氷から脱離したH2Oのオルソ／パラ比
キーワード：氷、オルソ／パラ比、核スピン、彗星、星間分子雲
Water has two nuclear-spin isomers: ortho- and para-H2O. Some observations of interstellar space and cometary comae have reported the existence of gaseous H2O molecules with anomalous ortho-to-para ratios (OPRs) less than the statistical value of three. This has been often used to estimate the formation temperature of ice on dust, which is inferred to be below 50 K. The use of the OPR as a temperature probe requires the assumption that the OPR of H2O desorbed from ice is related to the ice-formation temperature. However, the mechanism that determines the OPR of H2O desorbed from ice is unclear, and we still do not understand the origin of the anomalous OPRs measured for interstellar H2O. An important limiting factor is the lack of a laboratory study that defines the initial nuclear-spin state of H2O for the formation of ice at low temperatures.
The present study measures the OPR of H2O desorbed from ice made from para-H2O monomers at 11 K. The para-enrichment of H2O monomers is achieved in a solid Ne matrix (H2O/Ne = 1/1000) at 6 K. The Ne matrix is then warmed to 11 K to sublime Ne only, resulting in the formation of ice by the aggregation of para-H2O monomers. We perform direct measurements of the OPR of H2O desorbed from ice using rotationally resolved, resonance-enhanced multiphoton ionization spectroscopy. The photodesorbed H2O molecules from the ice have the statistical OPR value of three, demonstrating the immediate nuclear-spin state mixing of H2O towards the statistical value of ice even at 11 K. The OPR of H2O thermally desorbed from the ice also shows the expected statistical value. Our results indicate that the OPR of H2O desorbed from interstellar ice should be the statistical value regardless of the formation process of the ice, which cannot be used to deduce the ice-formation temperature. This study highlights the importance of interstellar gas-phase processes in understanding anomalous abundance ratios of nuclear-spin isomers of molecules in space.
Hama, T., Kouchi, A., & Watanabe, N. 2016, Science, 351, 65.
The present study measures the OPR of H2O desorbed from ice made from para-H2O monomers at 11 K. The para-enrichment of H2O monomers is achieved in a solid Ne matrix (H2O/Ne = 1/1000) at 6 K. The Ne matrix is then warmed to 11 K to sublime Ne only, resulting in the formation of ice by the aggregation of para-H2O monomers. We perform direct measurements of the OPR of H2O desorbed from ice using rotationally resolved, resonance-enhanced multiphoton ionization spectroscopy. The photodesorbed H2O molecules from the ice have the statistical OPR value of three, demonstrating the immediate nuclear-spin state mixing of H2O towards the statistical value of ice even at 11 K. The OPR of H2O thermally desorbed from the ice also shows the expected statistical value. Our results indicate that the OPR of H2O desorbed from interstellar ice should be the statistical value regardless of the formation process of the ice, which cannot be used to deduce the ice-formation temperature. This study highlights the importance of interstellar gas-phase processes in understanding anomalous abundance ratios of nuclear-spin isomers of molecules in space.
Hama, T., Kouchi, A., & Watanabe, N. 2016, Science, 351, 65.