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Impact induced motion of boulders and their effect on ejecta emplacement on rubble-pile targets

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URI: https://hdl.handle.net/10016/37249
DOI: https://doi.org/10.5194/epsc2022-131
UXXI: CC/0000033556
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impact_EPSC_2022.pdf (1.11 MB)
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2022
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Europlanet Society
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Abstract
Asteroids smaller than about 50 km in diameter are the result of the break-up of a larger parent body. They are often considered to be rubble-pile objects, aggregates held together only by self-gravity or small cohesive forces, and have highly heterogeneous surfaces. Recently, the artificial impact experiment (SCI) of JAXA's Hayabusa2 mission on the surface of asteroid Ryugu created a relatively large crater (~14 m diameter) despite the presence of large boulders close to the impact location...
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Proceeding of: Europlanet Science Congress 2022 (EPSC 2022), Palacio de Congresos de Granada, Spain, 18-23 September 2022
Keywords
Asteroids, Induced impacts
Bibliographic citation
Ormö, Jens, et al. Impact induced motion of boulders and their effect on ejecta emplacement on rubble-pile targets. Europlanet Science Congress, Granada 18-23 September 2022. In: EPSC abstracts, Vol. 16, EPSC2022-131, 2022. 4 p.
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