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Title:
Thermal evolution of Kuiper belt objects, with implications for cryovolcanism
Authors:
Desch, Steven J.; Cook, Jason C.; Doggett, T. C.; Porter, Simon B.
Affiliation:
AA(School of Earth and Space Exploration, Arizona State University, P.O. Box 871404, Tempe, AZ 85287-1404, USA), AB(Southwest Research Institute, 1050 Walnut St., Suite 300, Boulder, CO 80302, USA), AC(School of Earth and Space Exploration, Arizona State University, P.O. Box 871404, Tempe, AZ 85287-1404, USA), AD(School of Earth and Space Exploration, Arizona State University, P.O. Box 871404, Tempe, AZ 85287-1404, USA)
Publication:
Icarus, Volume 202, Issue 2, p. 694-714. (Icarus Homepage)
Publication Date:
08/2009
Origin:
ELSEVIER
DOI:
10.1016/j.icarus.2009.03.009
Bibliographic Code:
2009Icar..202..694D

Abstract

We investigate the internal thermal evolution of Kuiper belt objects (KBOs), small (radii <1000 km), icy (mean densities <2500kgm‑3) bodies orbiting beyond Neptune, focusing on Pluto's moon Charon in particular. Our calculations are time-dependent and account for differentiation. We review evidence for ammonia hydrates in the ices of KBOs, and include their effects on the thermal evolution. A key finding is that the production of the first melt, at the melting point of ammonia dihydrate, ≈176 K, triggers differentiation of rock and ice. The resulting structure comprises a rocky core surrounded by liquids and ice, enclosed within a >100-km thick undifferentiated crust of rock and ice. This structure is especially conducive to the retention of subsurface liquid, and bodies the size of Charon or larger (radii >600 km) are predicted to retain some subsurface liquid to the present day. We discuss the possibility that this liquid can be brought to the surface rapidly via self-propagating cracks. We conclude that cryovolcanism is a viable process expected to affect the surfaces of large KBOs including Charon.
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