Planetary science: Tectonic overturn on Enceladus

Details Planetary science: Tectonic overturn on Enceladus Planetary science: Tectonic overturn on Enceladus

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010natge...3...75h&link_type=abstract

Nature Geoscience, Volume 3, Issue 2, pp. 75-76 (2010).

Mathematics

Logic

3

Scientific paper

The south pole of Saturn's icy moon Enceladus is anomalously warm,
geologically youthful and cryovolcanically active. Episodic convective
overturn explains how the moon's modest sources of internal heat can be
channelled into intense geological activity.

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