Cassini Finds an Oxygen–Carbon Dioxide Atmosphere at Saturn’s Icy Moon Rhea

Author:

Teolis B. D.1,Jones G. H.23,Miles P. F.1,Tokar R. L.4,Magee B. A.1,Waite J. H.1,Roussos E.5,Young D. T.1,Crary F. J.1,Coates A. J.23,Johnson R. E.6,Tseng W.-L.6,Baragiola R. A.6

Affiliation:

1. Southwest Research Institute, Space Science and Engineering Division, 6220 Culebra Road, San Antonio, TX 78238, USA.

2. Mullard Space Science Laboratory, Department of Space and Climate Physics, University College London (UCL), Holmbury St. Mary, Dorking, Surrey RH5 6NT, UK.

3. The Centre for Planetary Sciences at UCL/Birkbeck, Gower Street, London WC1E 6BT, UK.

4. Los Alamos National Laboratory, Space Science and Applications, Los Alamos, NM 87545, USA.

5. Max-Planck-Institut für Sonnensystemforschung, Max-Planck-Strasse 2, 37191 Katlenburg-Lindau, Germany.

6. University of Virginia, Department of Materials Science and Engineering, 116 Engineer’s Way, Charlottesville, VA 22903, USA.

Abstract

Extraterrestrial Atmosphere The detection of oxygen in the atmospheres of Jupiter's icy moons, Europa and Ganymede, and the presence of this gas as the main constituent of the atmosphere that surrounds Saturn's rings, has suggested the possibility of oxygen atmospheres around the icy moons that orbit inside Saturn's magnetosphere. Using the Ion Neutral Mass Spectrometer onboard the Cassini spacecraft, Teolis et al. (p. 1813 , published online 25 November; see the Perspective by Cruikshank ) report the detection of a very tenuous oxygen and carbon dioxide atmosphere around Saturn's icy moon Rhea. As with other icy satellites, this atmosphere is maintained through the dissociation of surface molecules and ejection into the atmosphere as a result of Saturn's magnetospheric radiation.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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