211 Exploring the Third Zone: The Geology of Pluto, Charon, and the Kuiper Belt
Tuesday, 27 September 2016
1:30 PM - 5:30 PM
Mile High Ballroom 2A/3A
GEOPHYSICS OF THE PLUTO SYSTEM
Paper number: 211-5
Program: Technical Sessions
Time: 2:30 PM – 2:45 PM
Authors
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Carey M. LisseJohns Hopkins University, Laurel, MD
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Orkan UmurhanSpace Science Division, Moffett Field, CA
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William B. McKinnonDepartment of Earth and Planetary Sciences and McDonnell Center for the Space Sciences, Saint Louis, MO
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Jeffrey M. MooreSpace Science Division, Moffett Field, CA
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Paul M. SchenkUniversities Space Research Association, Houston, TX
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James H. RobertsJohns Hopkins University Applied Physics Laboratory, Laurel, MD
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Ross BeyerAmes Research Center, Moffet Field, CA
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Carver J. BiersonUniversity of California Santa Cruz, Santa Cruz, CA
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S. Alan SternBoulder, CO
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Cathy OlkinSouthwest Research Institute, Boulder, CO
Abstract
The Sputnik Planum basin on Pluto may be an ancient impact feature. It is now buried with several km of solid N2 ice. This ice has a young surface age and appears to be convecting [10,11], driven by heat leaking out of the silicate interior. Sputnik Planum’s location close to the tidal axis may be a result of loading-driven reorientation [12-14]. Such reorientation likely requires a subsurface ocean and is also consistent with a thick elastic ice shell at present [13].
[1] Stern et al. Science 2015 [2] Nimmo et al., Icarus in press [3] Bierson et al., LPSC 2016 [4] Canup, Science 2005 [5] Desch et al., Icarus 2015 [6] Moore et al., Science 2016 [7] Robuchon & Nimmo, Icarus 2011 [8] Hammond et al., GRL 2016 [9] Manga & Wang, GRL 2007 [10] McKinnon et al., Nature 2016 [11] Trowbridge et al., Nature 2016 [12] Hamilton, Fall AGU 2015 [13] Nimmo et al., LPSC 2016 [14] Keane et al., LPSC 2016
Geological Society of America Abstracts with Programs. Vol. 48, No. 7
doi: 10.1130/abs/2016AM-279362
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