Antipodal velocity for laboratory impact experiments on porous targets.
Project/Area Number |
22740300
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Research Category |
Grant-in-Aid for Young Scientists (B)
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Allocation Type | Single-year Grants |
Research Field |
Solid earth and planetary physics
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Research Institution | Fukushima National College of Technology |
Principal Investigator |
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Project Period (FY) |
2010 – 2011
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Project Status |
Completed (Fiscal Year 2011)
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Budget Amount *help |
¥1,560,000 (Direct Cost: ¥1,200,000、Indirect Cost: ¥360,000)
Fiscal Year 2011: ¥650,000 (Direct Cost: ¥500,000、Indirect Cost: ¥150,000)
Fiscal Year 2010: ¥910,000 (Direct Cost: ¥700,000、Indirect Cost: ¥210,000)
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Keywords | 惑星起源 / 進化 / 惑星探査 / 惑星起源、進化 / 宇宙科学 / 岩石・鉱物・鉱床学 |
Research Abstract |
The surface of asteroid 25143 Itokawa is covered with numerous boulders although gravity is very small compared with that of other asteroids previously observed from spacecraft. The bulk porosiy of Itokawa is~ 40%, which is larger than that of asteroid Eros. Impact experiments on porous targets were carried out, in order to investigate the relationship between the ejecta velocity and the porosity of the target on catastrophic disruption. The result shows that antipodal velocity is mainly dependent on the shock pressure attenuation of the target, and not so greatly on the porosity.
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Report
(3 results)
Research Products
(11 results)
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[Journal Article] Three dimensional Structure of HayabusaSamples : Origin and Evolution of Itokawa Regolith2010
Author(s)
A. Tsuchiyama1, M. Uesugi, T. Matsushima, T. Michikami, T. Kadono, T. Nakamura, K. Uesugi, T. Nakano, S. A. Sandford, R. Noguchi, T. Matsumoto, J. Matsuno, T. Nagano, Y. Imai, A. Takeuchi, Y. Suzuki, T. Ogami, J. Katagiri, M. Ebihara, T. R. Ireland, F. Ki
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Journal Title
Science
Volume: 333
Pages: 1125-1128
Related Report
Peer Reviewed
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