On the Formation of the Hemispheric Dichotomy of Enceladus

Details On the Formation of the Hemispheric Dichotomy of Enceladus On the Formation of the Hemispheric Dichotomy of Enceladus

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.2028h&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.2028

Physics

Scientific paper

We present three-dimensional models of Enceladus that demonstrate (1)
how localized active regions can result from brittle deformation, and
(2) how topography on the silicate core can modulate convection and
allow tectonic activity to be focused in one hemisphere.

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