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Measurements of Polyatomic Molecule Formation on an Icy Grain Analog Using Fast AtomsCarbon dioxide has been produced from the impact of a monoenergetic O(P-3) beam upon a surface cooled to 4.8 K and covered with a CO ice. Using temperature-programmed desorption and mass spectrometer detection, we have detected increasing amounts of CO2 formation with O(P-3) energies of 2, 5, 10, and 14 eV. This is the first measurement of polyatomic molecule formation on a surface with superthermal atoms. The goal of this work is to detect other polyatomic species, such as CH3OH, which can be formed under conditions that simulate the grain temperature, surface coverage, and superthermal atoms present in shock-heated circumstellar and interstellar regions.
Document ID
20060052456
Acquisition Source
Ames Research Center
Document Type
Conference Paper
Authors
Chutjian, A.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Madsunkov, S.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Shortt, B. J.
(Cork Inst. of Tech. Cork, Ireland)
MacAskill, J. A.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Darrach, M. R.
(Jet Propulsion Lab., California Inst. of Tech. Pasadena, CA, United States)
Date Acquired
August 23, 2013
Publication Date
August 1, 2006
Publication Information
Publication: Proceedings of the NASA Laboratory Astrophysics Workshop
Subject Category
Astrophysics
Distribution Limits
Public
Copyright
Public Use Permitted.
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