Charon tectonics

被引:28
作者
Beyer, Ross A. [1 ,2 ]
Nimmo, Francis [3 ]
McKinnon, William B. [4 ]
Moore, Jeffrey M. [2 ]
Binzel, Richard P. [5 ]
Conrad, Jack W.
Cheng, Andy [6 ]
Ennico, K. [2 ]
Lauer, Tod R. [7 ]
Olkin, C. B. [8 ]
Robbins, Stuart [8 ]
Schenk, Paul [9 ]
Singer, Kelsi [8 ]
Spencer, John R. [8 ]
Stern, S. Alan [8 ]
Weaver, H. A. [6 ]
Young, L. A. [8 ]
Zangari, Amanda M. [8 ]
机构
[1] SETI Inst, Sagan Ctr, 189 Berndardo Ave, Mountain View, CA 94043 USA
[2] NASA, Ames Res Ctr, Moffett Field, CA 94035 USA
[3] Univ Calif Santa Cruz, Santa Cruz, CA 95064 USA
[4] Washington Univ, St Louis, MO 63130 USA
[5] MIT, 77 Massachusetts Ave, Cambridge, MA 02139 USA
[6] Johns Hopkins Univ, Appl Phys Lab, Laurel, MD 20723 USA
[7] Natl Opt Astron Observ, Tucson, AZ 85719 USA
[8] Southwest Res Inst, Boulder, CO 80302 USA
[9] Lunar & Planetary Inst, Houston, TX 77058 USA
基金
美国国家航空航天局;
关键词
Pluto; Charon; Geological processes; Tectonics; Image processing; KUIPER-BELT OBJECTS; GIANT IMPACT ORIGIN; PLUTO; EVOLUTION; IMAGER;
D O I
10.1016/j.icarus.2016.12.018
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
New Horizons images of Pluto's companion Charon show a variety of terrains that display extensional tectonic features, with relief surprising for this relatively small world. These features suggest a global extensional areal strain of order 1% early in Charon's history. Such extension is consistent with the presence of an ancient global ocean, now frozen. (C) 2016 The Authors. Published by Elsevier Inc. This is an open access article under the CC BY license.
引用
收藏
页码:161 / 174
页数:14
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