Research on Characteristics of Hypervelocity Impact-Induced Ejecta in Rubble-Pile Targets

ZHANG Hongyu1, CHI Runqiang1, SUN Miao1, WANG Han1, PANG Baojun1, ZHANG He2

PDF(3343 KB)
PDF(3343 KB)
Journal of Deep Space Exploration ›› 2023, Vol. 10 ›› Issue (4) : 428-435. DOI: 10.15982/j.issn.2096-9287.2023.20230021
Special Issue:Monitoring of and Desense Against Near-Earth Asteroids
Special Issue:Monitoring of and Desense Against Near-Earth Asteroids

Research on Characteristics of Hypervelocity Impact-Induced Ejecta in Rubble-Pile Targets

  • ZHANG Hongyu1, CHI Runqiang1, SUN Miao1, WANG Han1, PANG Baojun1, ZHANG He2
Author information +
History +

Abstract

Kinetic impact deflection is a highly feasible and mature technique in the field of asteroid defense, and has been successfully implemented in related deep space exploration missions. However, a critical issue associated with this technology pertains to the optimization of momentum transfer during the impact process, as well as the evaluation of impact efficacy through analysis of ejecta observation data, for a diverse range of asteroid types. In this study, a target model composed of rubble-piles, constructed with varying proportions of boulder size and mass ratio, was developed and subsequently subjected to numerical simulations of hypervelocity impact of aluminum impactors. The impact of boulder size and mass proportion on the morphology of the ejecta was investigated, and the underlying mechanisms governing these effects were elucidated. The results of the investigation demonstrated that asymmetrical ejecta morphologies were produced as a result of the hypervelocity impact of aluminum impactors on rubble-pile targets, with ray-like ejecta emerging in the gaps between the boulders. The ray part of the ejecta has a larger eject angle, and the ray length and quantity are related to boulder diameter and mass ratio. Based on the rubble-pile target model established in this study, it was found that the maximum momentum of the ejecta produced in the opposite direction of the impact velocity was generated by large-diameter boulder targets. This paper can provide valuable reference for the selection of impact zones in future kinetic impact deflection missions.

Keywords

asteroid defense / rubble-pile structure / hypervelocity impact / impact-induced ejecta

Cite this article

Download citation ▾
ZHANG Hongyu, CHI Runqiang, SUN Miao, WANG Han, PANG Baojun, ZHANG He. Research on Characteristics of Hypervelocity Impact-Induced Ejecta in Rubble-Pile Targets. Journal of Deep Space Exploration, 2023, 10(4): 428‒435 https://doi.org/10.15982/j.issn.2096-9287.2023.20230021

References

[1] SCHMIDT N. Planetary defense:global collaboration for defending Earth from asteroids and comets[M]. Berlin:Springer,2018.
[2] GONG Z,LI M,CHEN C,et al. The frontier science and key technologies of asteroid monitoring and early warning,security defense and resource utilization[J]. Chinese Science Bulletin,2019,65(5):346-372.
[3] Jet Propulsion Laboratory. Discovery statistics[EB/OL]. (2020-05-15)[2023-02-16].https://cneos.jpl.nasa.gov/stats/.
[4] PITZ A,KAPLINGER B,VARDAXIS G,et al. Conceptual design of a hypervelocity asteroid intercept vehicle (HAIV) and its flight validation mission[J]. Acta Astronautica,2014,94(1):42-56.
[5] YAMAGUCHI K,PARK J H,GU X,et al. Orbital dynamics of gravity tractor spacecraft employing artificial halo orbit[J]. Acta Astronautica,2022,198:376-387.
[6] SPITALE J N. Asteroid hazard mitigation using the Yarkovsky effect[J]. Science,2002,296(5565):77.
[7] LI M,WANG Y,WANG Y,et al. Enhanced kinetic impactor for deflecting large potentially hazardous asteroids via maneuvering space rocks[J]. Scientific Reports,2020,10(1):8506.
[8] HOLSAPPLE K A,HOUSEN K R. Momentum transfer in asteroid impacts. I. theory and scaling[J]. Icarus,2012,221(2):875-887.
[9] CHENG A F,MICHEL P,JUTZI M,et al. Asteroid impact & deflection assessment mission:kinetic impactor[J]. Planetary and Space Science,2016,121:27-35.
[10] A'HEARN M F,BELTON M J S,DELAMERE W A,et al. Deep Impact:excavating comet Tempel 1[J]. Science,2005,310(5746):258-264.
[11] RICHARDSON J E,MELOSH H J,LISSE C M,et al. A ballistics analysis of the Deep Impact ejecta plume:determining Comet Tempel 1's gravity,mass,and density[J]. Icarus,2007,191(2):176-209.
[12] BENSCH F,MELNICK G J,NEUFELD D A,et al. Submillimeter wave astronomy satellite observations of Comet 9P/Tempel 1 and Deep Impact[J]. Icarus,2006,184(2):602-610.
[13] RIVKIN A S,CHABOT N L,STICKLE A M,et al. The double asteroid redirection test (DART):planetary defense investigations and requirements[J]. The Planetary Science Journal,2021,2(5):173.
[14] THOMAS C A, NAIDU S P, SCHEIRICH P, et al. Orbital period change of Dimorphos due to the DART kinetic impact[J]. Nature, 2023, 616(7957):448-451.
[15] SCHIRBER M. Spacecraft crash slows down asteroid orbit by 32 minutes[J]. Physics,2022,15:156.
[16] CHENG A F, AGRUSA H F, BARBEE B W, et al. Momentum transfer from the DART mission kinetic impact on asteroid Dimorphos[J]. Nature, 2023, 616(7957):457-460.
[17] HOUSEN K R,HOLSAPPLE K A. Experimental measurements of momentum transfer in hypervelocity collisions[C]//Proceedings of 46th Annual Lunar and Planetary Science Conference. Texas,USA:2015.
[18] RADUCAN S D,DAVISON T M,COLLINS G S. Ejecta distribution and momentum transfer from oblique impacts on asteroid surfaces[J]. Icarus,2022,374:114793.
[19] VEVERKA J,THOMAS P C,ROBINSON M,et al. Imaging of small-scale features on 433 Eros from NEAR:evidence for a complex regolith[J]. Science,2001,292(5516):484-488.
[20] FUJIWARA A,KAWAGUCHI J,YEOMANS D K,et al. The rubble-pile asteroid Itokawa as observed by Hayabusa[J]. Science,2006,312(5778):1330-1334.
[21] WADA K,ISHIBASHI K,KIMURA H,et al. Size of particles ejected from an artificial impact crater on asteroid 162173 Ryugu[J]. Astronomy & Astrophysics,2021,647:A43.
[22] 王亚林,刘鹏,吴辉阳,等. 碎石堆构造小行星表面地形分析与仿真验证[J]. 深空探测学报(中英文),2019,6(5):481-487.WANG Y L,LIU P,WU H Y,et al. Terrain analysis and simulation verification on rubble-pile-constructed asteroid surfaces[J]. Journal of Deep Space Exploration,2019,6(5):481-487.
[23] MAZROUEI S,DALY M,BARNOUIN O,et al. Distribution of boulders on asteroid 25143 itokawa[C]//Proceedings of 43rd Annual Lunar and Planetary Science Conference. Texas, USA:[s. n.],2012.
[24] RADUCAN S D,JUTZI M,ZHANG Y,et al. Reshaping and ejection processes on rubble-pile asteroids from impacts[J]. Astronomy & Astrophysics,2022,665:L10.
[25] STEINBERG D. Equation of state and strength properties of selected materials[M]. Livermore:Lawrence Livermore National Laboratory,1996.
[26] LAINE L, SANDVIK A. Derivation of mechanical properties for sand[C]//Proceedings of the 4th Asia-Pacific Conference on Shock and impact loads on structures, CI-Premier PTE LTD. Singapore:ANSYS Inc.,2001.
[27] YOKOYAMA T,NAGASHIMA K,NAKAI I,et al. Samples returned from the asteroid Ryugu are similar to Ivuna-type carbonaceous meteorites[J]. Science,2022,379(6634):eabn7850.
[28] POHL L,BRITT D T. Strengths of meteorites-an overview and analysis of available data[J]. Meteoritics & Planetary Science,2020,55(4):962-987.
[29] ROZEHNAL J,BROŽ M,NESVORNÝ D,et al. SPH simulations of high-speed collisions between asteroids and comets[J]. Icarus,2022,383:115064.
[30] SAITO T,KAIHO K,ABE A,et al. Numerical simulations of hypervelocity impact of asteroid/comet on the Earth[J]. International Journal of Impact Engineering,2006,33(1-12):713-722.
[31] OSINSKI G R,PIERAZZO E. Impact cratering:processes and products[M]. West Sussex, UK:Blackwell Publishing Ltd,2013.
[32] KUROSAWA K,OKAMOTO T,GENDA H. Hydrocode modeling of the spallation process during hypervelocity impacts:implications for the ejection of Martian meteorites[J]. Icarus,2018,301:219-234.
[33] SHUVALOV V. A mechanism for the production of crater rays[J]. Meteoritics & Planetary Science,2012,47(2):262-267.
[34] SABUWALA T,BUTCHER C,GIOIA G,et al. Ray systems in granular cratering[J]. Physical Review Letters,2018,120(26):264501.
[35] MELOSH H J. Impact ejection,spallation,and the origin of meteorites[J]. Icarus,1984,59(2):234-260.
[36] DELLER J,LOWRY S,PRICE M,et al. SPH simulations of impacts on rubble pile asteroids[C]//Proceedings of European Planetary Science Congress. UK:[s. n.]:2013.
[37] MOROTA T,SUGITA S,CHO Y,et al. Sample collection from asteroid (162173) Ryugu by Hayabusa2:implications for surface evolution[J]. Science,2020,368(6491):654-659.
[38] ORMÖ J,RADUCAN S D,JUTZI M,et al. Boulder exhumation and segregation by impacts on rubble-pile asteroids[J]. Earth and Planetary Science Letters,2022,594:117713.
PDF(3343 KB)

Accesses

Citations

Detail

Sections
Recommended

/