IR Detection of H2O2 at 80 K in Ion-Irradiated Laboratory Ices Relevant to Europa

By M. Moore, R. Hudson. 2000

169 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science, Environmental Chemistry

View Paper: https://www.semanticscholar.org/paper/18a2df0ed3a46a5d681075aed5ca348d8af17f6a

How researchers see this paper

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In Astronomy and Astrophysics

1. E. V. van Dishoeck
2. J. Jørgensen
3. Y. Bénilan
4. H. Cottin
5. T. Bartels-Rausch
6. M. Palumbo
7. S. Bisschop
8. M. Moore

In Atmospheric Science

1. E. V. van Dishoeck
2. Y. Bénilan
3. H. Cottin
4. T. Bartels-Rausch
5. M. Palumbo
6. M. Moore
7. D. Jewitt
8. S. Bisschop

In Environmental Chemistry

1. Y. Bénilan
2. H. Cottin
3. T. Bartels-Rausch
4. M. Palumbo
5. M. Moore

Citations in the corpus

• Ice structures, patterns, and processes: A view across the icefields (2012, background): “Laboratory experiments also suggest a patchy distribution of H2O2 on Europa.”
• Temperature Dependence of the Formation of Hydrogen, Oxygen, and Hydrogen Peroxide in Electron-Irradiated Crystalline Water Ice (2006, background): “Moore and Hudson (2000) carried out infrared spectroscopy studies of the formation of hydrogen peroxide in water ice irradiated with 0.8 MeV protons at temperatures relevant to the icy Galilean satellites (80– 150 K).”
• Formation of compact solid water after ion irradiation at 15 K (2006, background): “It is well known that ion irradiation of pure solid H2O causes the formation of H2O2, H2, OH, and O2 (e.g., Johnson 1990; Moore & Hudson 2000; Baragiola et al. 2003; Gomis et al. 2004), thus some blank experiments are necessary to verify that the results discussed above are due to a change in the…”
• Europa’s Surface Composition (2009, result): “These results are also in general agreement with the ion irradiation measurements of Moore and Hudson (2000) and Gomis et al. (2004a,b), although Moore and Hudson (2000) found that the addition of electron scavengers such CO2 increased the yield at Europa-like temperatures and may explain the…”
• Testing grain-surface chemistry in massive hot-core regions (2007, background): “Laboratory experiments show that beyond a certain minimum dose of irradiation the reaction products often do reach a constant plateau (Gerakines et al. 1996; Moore & Hudson 2000; van Broekhuizen et al. 2004; Hagen et al. 1979).”
• Photodestruction of Relevant Interstellar Molecules in Ice Mixtures (2003, methodology): “Ice Preparation and Analysis The experimental setup has been described in detail by Hudson & Moore (1995) and Moore & Hudson (1998, 2000).”