Volume 42 Issue 3
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Article Navigation >  Chinese Journal of Space Science  > 2022  >  42(3): 463-475
ZHOU Qi, ZHENG Jianhua, LI Mingtao. Analysis of Sensitive Parameters of Momentum Transfer Factor in Kinetic Impact Defending Small Bodies (in Chinese). Chinese Journal of Space Science, 2022, 42(3): 463-475. DOI: 10.11728/cjss2022.03.210126013
Citation: ZHOU Qi, ZHENG Jianhua, LI Mingtao. Analysis of Sensitive Parameters of Momentum Transfer Factor in Kinetic Impact Defending Small Bodies (in Chinese). Chinese Journal of Space Science, 2022, 42(3): 463-475. DOI: 10.11728/cjss2022.03.210126013
shu

Analysis of Sensitive Parameters of Momentum Transfer Factor in Kinetic Impact Defending Small Bodies

doi: 10.11728/cjss2022.03.210126013 cstr: 32142.14.cjss2022.03.210126013

  • National Space Science Center, Chinese Academy of Sciences, Beijing 100190

  • University of Chinese Academy of Sciences, Beijing 100049

  • Received Date: 2021-01-26
  • Accepted Date: 2021-09-26
  • Rev Recd Date: 2022-02-04
    • Available Online: 2022-05-26
    Abstract
  • Momentum transfer factor β is the key factor to evaluate effect of kinetic impact. In this paper, theoretical model of momentum transfer factor in kinetic impact is investigated, as well as the influence of impactor properties and small body structure properties on the factor. Meanwhile, the crater effect and momentum transfer factor of small bodies with different kinetic impact schemes and structural characteristics are studied. Results show that scaling law parameter μ, a coefficient related to strength properties of target material which is obtained by ground experiment fitting, has a great effect on the factor. The velocity/density of impactor and density/surface strength of small body have a great effect on the factor for small body with a single rock structure, while radius of impactor and gravity of small body have a small effect. In the meantime, the value of β is significant. The factor is insensitive to parameters of impactor properties and small body structure properties for small body with a rubble-pile structure, and its value is close to 1. The formation of crater and momentum transfer factor in three different kinetic impact schemes indicates that the initial kinetic energy of impactor has a great influence on the factor. In the same kinetic impact scheme where gravity dominates the crater formation, the momentum transfer factor of a C-complex asteroid is largest followed by S-complex and X-complex. However, when strength dominates crater formation, the factors of all complexes are smaller and basically the same.

     

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