Journal
PLANETARY AND SPACE SCIENCE
Volume 107, Issue -, Pages 77-83Publisher
PERGAMON-ELSEVIER SCIENCE LTD
DOI: 10.1016/j.pss.2014.10.006
Keywords
Asteroids; Fragmentation; Collisions; Internal structure; Gravitational aggregates
Categories
Funding
- NASA Planetary Geology & Geophysics program [NNX11AP22G]
- extinct [AYA2011-30106-C02-02]
- Spanish Ministry of Education, Culture and Sports [PRX12/00129]
- Space Plasma Laboratory, ISAS, JAXA
- NASA [137946, NNX11AP22G] Funding Source: Federal RePORTER
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We conducted impact experiments at the NASA Ames Vertical Gun Range in the context of an ongoing set of experiments to investigate both target shape and impact speed effects on fragment shapes and mass-frequency distributions in collisions on basalt targets. In this work we present the first part of that set, regarding mostly target shape effects. We impacted both irregularly-shaped and spherical basalt targets at speeds ranging from 4-6 km/s. We obtained mass-frequency distributions from fragments recovered from the impact chamber and measured fragments shapes using a combination of image analysis and manual measurements with a caliper. We find that the characteristics of the massfrequency distributions and the range of fragment shapes show no significant dependence on target shape (i.e., flat, 'shell-like' fragments are produced in impacts into irregularly-shaped targets as well as spherical ones). We note that many thin, plate-like impact fragments seem to originate from lowerspeed impacts and can originate from the interior of the targets (in addition to the flattened fragments often seen to origin from the near-surface spall zone in cratering impacts). We measure the porosity of aggregates made by artificially (but randomly) reassembling fragments from each impact to be on the order of 50%, significantly larger than that for hexagonal lattice and random packing of equal sized spheres. (C) 2014 Elsevier Ltd. All rights reserved.
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