Published March 20, 2006 | Version Supplemental Material
Journal Article Open

Cassini Observes the Active South Pole of Enceladus

Abstract

Cassini has identified a geologically active province at the south pole of Saturn's moon Enceladus. In images acquired by the Imaging Science Subsystem (ISS), this region is circumscribed by a chain of folded ridges and troughs at ∼55°S latitude. The terrain southward of this boundary is distinguished by its albedo and color contrasts, elevated temperatures, extreme geologic youth, and narrow tectonic rifts that exhibit coarse-grained ice and coincide with the hottest temperatures measured in the region. Jets of fine icy particles that supply Saturn's E ring emanate from this province, carried aloft by water vapor probably venting from subsurface reservoirs of liquid water. The shape of Enceladus suggests a possible intense heating epoch in the past by capture into a 1:4 secondary spin/orbit resonance.

Additional Information

© 2006 American Association for the Advancement of Science. 25 November 2005; accepted 21 February 2006. We acknowledge the financial support of NASA/JPL, the UK Particle Physics and Astronomy Research Council, the Deutsches Zentrum fur Luft- und Raumfahrt (German Aerospace Center), and Université Paris VII Denis Diderot, Commissariat à l'Énergie Atomique, Astrophysique Interactions Multieschelle, France.

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Additional details

Identifiers

Eprint ID
36593
DOI
10.1126/science.1123013
Resolver ID
CaltechAUTHORS:20130125-103250989

Related works

Funding

NASA
JPL
Particle Physics and Astronomy Research Council (PPARC)
Deutsches Zentrum fur Luft- und Raumfahrt (DLR)
Commissariat à l'Energie Atomique (CEA)

Dates

Created
2013-01-25
Created from EPrint's datestamp field
Updated
2021-11-09
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Caltech Custom Metadata

Caltech groups
Division of Geological and Planetary Sciences (GPS)