NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Laboratory IR Detection of H2O, CO2 in Ion-Irradiated Ices Relevant to EuropaHydrogen peroxide has been identified on Europa (Carlson et al. 1999) based in part on the 3.50 micron absorption feature observed in Galileo NIMS spectra. The observed feature was fitted with laboratory reflectance spectra of H2O + H2O2. Since condensed phase molecules on Europa (H2O, CO2, SO2, and H2O2) are bombarded with a significant flux of energetic particles (H(+), O(n+), S(n+) and e-), we examined the proton irradiation of H2O at 80 K and the conditions for the IR detection of H2O2 near 3.5 microns. Contrary to expectations, H2O2 was not detected if pure H2O ice was irradiated at 80 K. This was an unexpected result since, H2O2 was detected if pure H2O was irradiated at 18 K. We find, however, that if H2O ice contains either O2 or CO2 then H2O2 is detected after irradiation at 80 K (Moore and Hudson, 1999). The source of O2 for the H2O ice on Europa could come from surface interactions with the tenuous oxygen atmosphere, or from the bombardment of the surface by O(n+).
Document ID
19990115745
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
Moore, Marla H.
(NASA Goddard Space Flight Center Greenbelt, MD United States)
Hudson, R. L.
(NASA Goddard Space Flight Center Greenbelt, MD United States)
Date Acquired
August 19, 2013
Publication Date
January 1, 1999
Subject Category
Lunar And Planetary Exploration
Meeting Information
Meeting: Division of Planetary Sciences
Location: Padua
Country: Italy
Start Date: October 10, 1999
End Date: October 15, 1999
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

Available Downloads

There are no available downloads for this record.
No Preview Available