TY - JOUR
T1 - Radiation chemistry in ammonia-water ices
AU - Loeffler, M. J.
AU - Raut, U.
AU - Baragiola, R. A.
N1 - Funding Information:
This research was supported by Grant No. NNX07AL48G from NASA Outer Planet Research and Grant No. NNX08AMB6G from Planetary Geology and Geophysics programs. We thank Dr. J-H. Kim for calibration of the beam current monitor.
PY - 2010
Y1 - 2010
N2 - We studied the effects of 100 keV proton irradiation on films of ammonia-water mixtures between 20 and 120 K. Irradiation destroys ammonia, leading to the formation and trapping of H2, N2, NO, and N2 O, the formation of cavities containing radiolytic gases, and ejection of molecules by sputtering. Using infrared spectroscopy, we show that at all temperatures the destruction of ammonia is substantial, but at higher temperatures (120 K), it is nearly complete (∼97% destroyed) after a fluence of 1016 ions/cm2. Using mass spectroscopy and microbalance gravimetry, we measure the sputtering yield of our sample and the main components of the sputtered flux. We find that the sputtering yield depends on fluence. At low temperatures, the yield is very low initially and increases quadratically with fluence, while at 120 K the yield is constant and higher initially. The increase in the sputtering yield with fluence is explained by the formation and trapping of the ammonia decay products, N2 and H 2, which are seen to be ejected from the ice at all temperatures.
AB - We studied the effects of 100 keV proton irradiation on films of ammonia-water mixtures between 20 and 120 K. Irradiation destroys ammonia, leading to the formation and trapping of H2, N2, NO, and N2 O, the formation of cavities containing radiolytic gases, and ejection of molecules by sputtering. Using infrared spectroscopy, we show that at all temperatures the destruction of ammonia is substantial, but at higher temperatures (120 K), it is nearly complete (∼97% destroyed) after a fluence of 1016 ions/cm2. Using mass spectroscopy and microbalance gravimetry, we measure the sputtering yield of our sample and the main components of the sputtered flux. We find that the sputtering yield depends on fluence. At low temperatures, the yield is very low initially and increases quadratically with fluence, while at 120 K the yield is constant and higher initially. The increase in the sputtering yield with fluence is explained by the formation and trapping of the ammonia decay products, N2 and H 2, which are seen to be ejected from the ice at all temperatures.
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U2 - 10.1063/1.3308484
DO - 10.1063/1.3308484
M3 - Article
AN - SCOPUS:76349096055
SN - 0021-9606
VL - 132
JO - Journal of Chemical Physics
JF - Journal of Chemical Physics
IS - 5
M1 - 054508
ER -