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冥卫构造

Charon tectonics.

作者信息

Beyer Ross A, Nimmo Francis, McKinnon William B, Moore Jeffrey M, Binzel Richard P, Conrad Jack W, Cheng Andy, Ennico K, Lauer Tod R, Olkin C B, Robbins Stuart, Schenk Paul, Singer Kelsi, Spencer John R, Stern S Alan, Weaver H A, Young L A, Zangari Amanda M

机构信息

Sagan Center at the SETI Institute, 189 Berndardo Ave, Mountain View, California 94043, USA.

NASA Ames Research Center, Moffet Field, CA 94035-0001, USA.

出版信息

Icarus. 2017 May 1;287:161-174. doi: 10.1016/j.icarus.2016.12.018. Epub 2016 Dec 16.

DOI:10.1016/j.icarus.2016.12.018
PMID:28919640
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC5599803/
Abstract

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.

摘要

“新视野号”对冥王星的卫星卡戎拍摄的图像显示出了各种各样的地形，这些地形呈现出伸展构造特征，对于这个相对较小的天体来说，其地形起伏令人惊讶。这些特征表明，在卡戎历史早期，全球伸展区域应变约为1%。这种伸展与现在已冻结的古老全球海洋的存在是一致的。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/05d7a1ff8aef/nihms857809f20.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/044cff73b618/nihms857809f1.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/9b6f42dcf637/nihms857809f2.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/6582971f90a2/nihms857809f3.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/ba7722d889e5/nihms857809f4.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/246c88ec9891/nihms857809f5.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/ed890816f62c/nihms857809f6.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/5a12d9351693/nihms857809f7.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/217053b576d3/nihms857809f8.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/80e38a900f30/nihms857809f9.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/de617517c267/nihms857809f10.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/9ca150f47093/nihms857809f11.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/68e1958f5142/nihms857809f12.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/48e1872cdfb4/nihms857809f13.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/a126932d44a4/nihms857809f14.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/8a13bde2cb18/nihms857809f15.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/ae1887161c56/nihms857809f16.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/7ac5e8884a61/nihms857809f17.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/fca86b9d0459/nihms857809f18.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/59129292cf03/nihms857809f19.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/05d7a1ff8aef/nihms857809f20.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/044cff73b618/nihms857809f1.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/9b6f42dcf637/nihms857809f2.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/6582971f90a2/nihms857809f3.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/ba7722d889e5/nihms857809f4.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/246c88ec9891/nihms857809f5.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/ed890816f62c/nihms857809f6.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/5a12d9351693/nihms857809f7.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/217053b576d3/nihms857809f8.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/80e38a900f30/nihms857809f9.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/de617517c267/nihms857809f10.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/9ca150f47093/nihms857809f11.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/68e1958f5142/nihms857809f12.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/48e1872cdfb4/nihms857809f13.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/a126932d44a4/nihms857809f14.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/8a13bde2cb18/nihms857809f15.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/ae1887161c56/nihms857809f16.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/7ac5e8884a61/nihms857809f17.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/fca86b9d0459/nihms857809f18.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/59129292cf03/nihms857809f19.jpg
https://cdn.ncbi.nlm.nih.gov/pmc/blobs/172b/5599803/05d7a1ff8aef/nihms857809f20.jpg

相似文献

1
Charon tectonics.冥卫构造
Icarus. 2017 May 1;287:161-174. doi: 10.1016/j.icarus.2016.12.018. Epub 2016 Dec 16.
2
The formation of Charon's red poles from seasonally cold-trapped volatiles.从季节性冷阱挥发物形成冥卫一的红色极区。
Nature. 2016 Nov 3;539(7627):65-68. doi: 10.1038/nature19340. Epub 2016 Sep 14.
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The geology of Pluto and Charon through the eyes of New Horizons.新视野号眼中的冥王星和卡戎的地质特征。
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Evidence for crystalline water and ammonia ices on Pluto's satellite charon.冥王星的卫星卡戎上存在结晶水和氨冰的证据。
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A giant impact origin for Pluto's small moons and satellite multiplicity in the Kuiper belt.冥王星小卫星的巨大撞击起源与柯伊伯带中的卫星多样性
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引用本文的文献

1
Endogenically sourced volatiles on Charon and other Kuiper belt objects.冥卫一（卡戎）及其他柯伊伯带天体上的内源挥发性物质。
Nat Commun. 2022 Aug 9;13(1):4457. doi: 10.1038/s41467-022-31846-8.
2
Charon's refractory factory.
Sci Adv. 2022 Jun 17;8(24):eabq5701. doi: 10.1126/sciadv.abq5701.

本文引用的文献

1
The formation of Charon's red poles from seasonally cold-trapped volatiles.从季节性冷阱挥发物形成冥卫一的红色极区。
Nature. 2016 Nov 3;539(7627):65-68. doi: 10.1038/nature19340. Epub 2016 Sep 14.
2
Surface compositions across Pluto and Charon.冥王星和卡戎表面的成分。
Science. 2016 Mar 18;351(6279):aad9189. doi: 10.1126/science.aad9189.
3
The geology of Pluto and Charon through the eyes of New Horizons.新视野号眼中的冥王星和卡戎的地质特征。
Science. 2016 Mar 18;351(6279):1284-93. doi: 10.1126/science.aad7055.
4
The Pluto system: Initial results from its exploration by New Horizons.冥王星系统：新视野号对其的探索的初步结果。
Science. 2015 Oct 16;350(6258):aad1815. doi: 10.1126/science.aad1815.
5
A giant impact origin of Pluto-Charon.冥王星-卡戎的巨大撞击起源。
Science. 2005 Jan 28;307(5709):546-50. doi: 10.1126/science.1106818.