skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: Photolysis of solid NH{sub 3} and NH{sub 3}-H{sub 2}O mixtures at 193 nm

Journal Article · · Journal of Chemical Physics
DOI:https://doi.org/10.1063/1.3506577· OSTI ID:21559957
 [1];  [2]
  1. Astrochemistry Laboratory, NASA Goddard Space Flight Center, Code 691, Greenbelt, Maryland 20771 (United States)
  2. Laboratory for Atomic and Surface Physics, Engineering Physics, University of Virginia, Charlottesville, Virginia 22904 (United States)

We have studied UV photolysis of solid ammonia and ammonia-dihydrate samples at 40 K, using infrared spectroscopy, mass spectrometry, and microgravimetry. We have shown that in the pure NH{sub 3} sample, the main species ejected are NH{sub 3}, H{sub 2}, and N{sub 2}, where the hydrogen and nitrogen increase with laser fluence. This increase in N{sub 2} ejection with laser fluence explains the increase in mass loss rate detected by a microbalance. In contrast, for the ammonia-water mixture, we see very weak signals of H{sub 2} and N{sub 2} in the mass spectrometer, consistent with the very small mass loss during the experiment and with a <5% decrease in the NH{sub 3} infrared absorption bands spectroscopy after a fluence of {approx}3 x 10{sup 19} photons/cm{sup 2}. The results imply that ammonia-ice mixtures in the outer solar system are relatively stable under solar irradiation.

OSTI ID:
21559957
Journal Information:
Journal of Chemical Physics, Vol. 133, Issue 21; Other Information: DOI: 10.1063/1.3506577; (c) 2010 American Institute of Physics; ISSN 0021-9606
Country of Publication:
United States
Language:
English