Numerical simulation of impact cratering on granular material
A new numerical code based on the Distinct Element Method (DEM) is developed to study the impact cratering processes on granular material. This code has a potential advantage to simulate the cratering process on granular material, since the movement of discrete particles can be treated. To show the...
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| Published in | Icarus (New York, N.Y. 1962) Vol. 180; no. 2; pp. 528 - 545 |
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| Main Authors | , , |
| Format | Journal Article |
| Language | English |
| Published |
San Diego, CA
Elsevier Inc
01.02.2006
Elsevier |
| Subjects | |
| Online Access | Get full text |
| ISSN | 0019-1035 1090-2643 |
| DOI | 10.1016/j.icarus.2005.10.002 |
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| Abstract | A new numerical code based on the Distinct Element Method (DEM) is developed to study the impact cratering processes on granular material. This code has a potential advantage to simulate the cratering process on granular material, since the movement of discrete particles can be treated. To show the physical plausibility of this code, we conduct 3-D numerical simulations of vertical impact into granular material targets that consist of 384,000 particles, and compare the results with those from experimental studies. It is shown that the excavation stage of cratering derived from experimental studies is represented well by our simulation: the size of the crater cavity, and the ejecta velocity and angle distributions are consistent with those obtained in laboratory experiments. The impact simulation code developed in this study is thus suggested to be useful for the analysis of the impact cratering process on granular material. |
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| AbstractList | A new numerical code based on the Distinct Element Method (DEM) is developed to study the impact cratering processes on granular material. This code has a potential advantage to simulate the cratering process on granular material, since the movement of discrete particles can be treated. To show the physical plausibility of this code, we conduct 3-D numerical simulations of vertical impact into granular material targets that consist of 384,000 particles, and compare the results with those from experimental studies. It is shown that the excavation stage of cratering derived from experimental studies is represented well by our simulation: the size of the crater cavity, and the ejecta velocity and angle distributions are consistent with those obtained in laboratory experiments. The impact simulation code developed in this study is thus suggested to be useful for the analysis of the impact cratering process on granular material. |
| Author | Senshu, Hiroki Wada, Koji Matsui, Takafumi |
| Author_xml | – sequence: 1 givenname: Koji surname: Wada fullname: Wada, Koji email: wada@neko.lowtem.hokudai.ac.jp organization: Department of Complexity Science and Engineering, Graduate School of Frontier Sciences, University of Tokyo, 5-1-5, Kashiwanoha, Kashiwa-shi, Chiba 277-8561, Japan – sequence: 2 givenname: Hiroki surname: Senshu fullname: Senshu, Hiroki email: senshu@jamstec.go.jp organization: Institute for Research on Earth Evolution, Japan Agency for Marine–Earth Science and Technology, 2-15, Natsushima-cho, Yokosuka 237-0061, Japan – sequence: 3 givenname: Takafumi surname: Matsui fullname: Matsui, Takafumi email: matsui@k.u-tokyo.ac.jp organization: Department of Complexity Science and Engineering, Graduate School of Frontier Sciences, University of Tokyo, 5-1-5, Kashiwanoha, Kashiwa-shi, Chiba 277-8561, Japan |
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| Keywords | Impact processes Cratering Computer techniques Granular materials Digital simulation Impact phenomena Velocity distribution Solar system Experimental study |
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| SubjectTerms | Astronomy Computer techniques Cratering Earth, ocean, space Exact sciences and technology Impact processes Solar system |
| Title | Numerical simulation of impact cratering on granular material |
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