MESOSCALE MODELLING OF THE COMPACTION OF WATER-RICH ASTEROIDS BY LOW-VELOCITY IMPACTS

被引：0

作者：

Davison, T. M. ^{[1
]}

Collins, G. S. ^{[1
]}

Bland, P. A. ^{[2
]}

Derrick, J. G. ^{[1
]}

Ciesla, F. J. ^{[3
]}

机构：

[1] Imperial Coll London, Dept Earth Sci & Engn, Impacts Astromat Res Ctr, London SW7 2AZ, England

[2] Curtin Univ, Dept Appl Geol, GPO Box U1987, Perth, WA 6845, Australia

[3] Univ Chicago, Dept Geophys Sci, 5734 South Ellis Ave, Chicago, IL 60637 USA

来源：

METEORITICS & PLANETARY SCIENCE | 2016年 / 51卷

关键词：

D O I：

暂无

中图分类号：

P3 [地球物理学]; P59 [地球化学];

学科分类号：

0708 ; 070902 ;

摘要：

引用

页码：A222 / A222

页数：1

共 5 条

[1]

Amsden A A., 1980, A simplified ALE computer program for fluid flow at all speeds

[2] Pressure-temperature evolution of primordial solar system solids during impact-induced compaction [J].

Bland, P. A. ;

Collins, G. S. ;

Davison, T. M. ;

Abreu, N. M. ;

Ciesla, F. J. ;

Muxworthy, A. R. ;

Moore, J. .

NATURE COMMUNICATIONS, 2014, 5

[3] Propagation of impact-induced shock waves in porous sandstone using mesoscale modeling [J].

Gueldemeister, Nicole ;

Wuennemann, Kai ;

Durr, Nathanael ;

Hiermaier, Stefan .

METEORITICS & PLANETARY SCIENCE, 2013, 48 (01) :115-133

[4] Thickness of a European ice shell from impact crater simulations [J].

Turtle, EP ;

Pierazzo, E .

SCIENCE, 2001, 294 (5545) :1326-1328

[5] A strain-based porosity model for use in hydrocode simulations of impacts and implications for transient crater growth in porous targets [J].

Wünnemann, K ;

Collins, GS ;

Melosh, HJ .

ICARUS, 2006, 180 (02) :514-527

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