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Title:
Detection of an oxygen atmosphere on Jupiter's moon Europa
Authors:
Hall, D. T.; Strobel, D. F.; Feldman, P. D.; McGrath, M. A.; Weaver, H. A.
Publication:
Nature, Volume 373, Issue 6516, pp. 677-679 (1995). (Nature Homepage)
Publication Date:
02/1995
Origin:
NATURE
DOI:
10.1038/373677a0
Bibliographic Code:
1995Natur.373..677H

Abstract

EUROPA, the second large satellite out from Jupiter, is roughly the size of Earth's Moon, but unlike the Moon, it has water ice on its surface1. There have been suggestions that an oxygen atmosphere should accumulate around such a body, through reactions which break up the water molecules and form molecular hydrogen and oxygen2,3. The lighter H2 molecules would escape from Europa relatively easily, leaving behind an atmosphere rich in oxygen. Here we report the detection of atomic oxygen emission from Europa, which we interpret as being produced by the simultaneous dissociation and excitation of atmospheric O2 by electrons from Jupiter's magnetosphere. Europa's molecular oxygen atmosphere is very tenuous, with a surface pressure about 10-11 that of the Earth's atmosphere at sea level.
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