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Water vapor can be formed in gas phase and on the ice mantles of dust grains (see “Water in the Universe”). Once formed, the molecule is mainly destroyed by photodissociation through the effect of UV photons. In gas phase the molecule can be formed in low-temperature clouds through the chain of reactions:
In this set of reactions, H2 is formed on the surface of dust grains, and H3 +is the product of the reaction...
References
van Dishoeck EF, Herbst E, Neufeld DA (2013) Interstellar water chemistry: from laboratory to observations. Chem Rev 113:9045–9085
van Dishoeck EF, Bergin EA, Lis DC, Lunine JI (2014) Water: from clouds to planets. In: Beuther H, Klessen R, Dullemond C, Henning T (eds) Protostars and planets VI. University of Arizona Press, Tucson, in press
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Quintanilla, J.C. (2014). Water, Formation and Photodissociation. In: Amils, R., et al. Encyclopedia of Astrobiology. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-642-27833-4_5277-1
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DOI: https://doi.org/10.1007/978-3-642-27833-4_5277-1
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Publisher Name: Springer, Berlin, Heidelberg
Online ISBN: 978-3-642-27833-4
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Latest
Water, Formation and Photodissociation- Published:
- 16 March 2023
DOI: https://doi.org/10.1007/978-3-642-27833-4_5277-2
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Water, Formation and Photodissociation- Published:
- 18 April 2015
DOI: https://doi.org/10.1007/978-3-642-27833-4_5277-1