Hydrogen peroxide on the surface of Europa.
Spatially resolved infrared and ultraviolet wavelength spectra of Europa's leading, anti-jovian quadrant observed from the Galileo spacecraft show absorption features resulting from hydrogen peroxide. Comparisons with laboratory measurements indicate surface hydrogen peroxide concentrations of about 0.13 percent, by number, relative to water ice. The inferred abundance is consistent with radiolytic production of hydrogen peroxide by intense energetic particle bombardment and demonstrates that Europa's surface chemistry is dominated by radiolysis.
Carlson
R W
RW
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA. rcarlson@lively.jpl.nasa.gov
Anderson
M S
MS
Johnson
R E
RE
Smythe
W D
WD
Hendrix
A R
AR
Barth
C A
CA
Soderblom
L A
LA
Hansen
G B
GB
McCord
T B
TB
Dalton
J B
JB
Clark
R N
RN
Shirley
J H
JH
Ocampo
A C
AC
Matson
D L
DL
D005118:Extraterrestrial Environment; D006861:Hydrogen Peroxide / Q000032:analysis* / Q000737:chemistry; D007053:Ice; D018538:Jupiter; D013055:Spectrophotometry, Infrared; D013056:Spectrophotometry, Ultraviolet; D014867:Water / Q000737:chemistry
D007053:Ice; D014867:Water; D006861:Hydrogen Peroxide