Numerical simulation of impact crater formation and distribution of high-pressure polymorphs

被引:16
作者
Lv, He [1 ]
He, Qiguang [1 ]
Chen, Xiaowei [1 ]
Han, Pengfei [1 ]
机构
[1] Beijing Inst Technol, State Key Lab Explos Sci & Technol, Beijing 100081, Peoples R China
基金
中国国家自然科学基金;
关键词
FE-SPH adaptive Method; Planetary sciences; Impact craters; Numerical simulation; Polymorphs; HYPERVELOCITY IMPACTS; BALLISTIC LIMIT; VELOCITY IMPACT; COESITE; PROTECTION; METAMORPHISM; TRANSITION; MORPHOLOGY; PARTICLES; SANDSTONE;
D O I
10.1016/j.actaastro.2022.11.048
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
Understanding the formation of impact craters on planetary surfaces has fundamental importance in geology, impact dynamics, and planetary sciences. The finite element-smoothed particle hydrodynamics (FE-SPH) adaptive method combines the advantages of smoothed particle hydrodynamics (SPH) and finite element method (FEM) in solving hypervelocity impact (HVI) problems. Employing FE-SPH adaptive method is a new idea for the analysis of planetary impact cratering which is different from impact-simplified arbitrary Lagrangian Eulerian (iSALE). In this paper, we establish a complete numerical model of planetary impact cratering through the FESPH method, including material failure criterion, thermodynamic analysis, gravity preloading, etc. We reproduce the numerical results by Collins et al. (2012) and highly consistent results are obtained through comparative analysis. This study simulates the formation process of simple and complex impact craters, and the temperature, pressure, density, and geometric shape of the impact zone can be quantitatively obtained. We further analyze the distribution of polymorphs and rock fragmentations in the impact zone based on the theories of shock metamorphism. The proposed analysis method may assist geologists in conducting geological studies.
引用
收藏
页码:169 / 186
页数:18
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