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Updated: Aug 2, 2026

Kinematic History of a Salient-recess Junction Explored through a Combined Approach of Field Data and Analog Sandbox Modeling
06:55

Kinematic History of a Salient-recess Junction Explored through a Combined Approach of Field Data and Analog Sandbox Modeling

Published on: August 5, 2016

イオの山の起源は,推力断層と大規模な質量移動によるものです

Schenk1, Bulmer

  • 1P. M. Schenk, Lunar and Planetary Institute, Houston, TX 77058, USA. M. H. Bulmer, Center for Earth and Planetary Science, National Air and Space Museum, Washington, DC 20560, USA.

Science (New York, N.Y.)
|March 21, 1998
PubMed
まとめ

イオのユーベア・モンテス山は,地殻の10.5kmの上昇と傾きによって形成されました. これは,巨大な斜面の故障を引き起こし,太陽系の最大の破片のエプロンの1つを生み出しました.

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