|Appears in Collections:||Biological and Environmental Sciences Journal Articles|
|Peer Review Status:||Refereed|
|Title:||Fragment shapes in impact experiments ranging from cratering to catastrophic disruption|
|Citation:||Michikami T, Hagermann A, Kadokawa T, Yoshida A, Shimada A, Hasegawa S & Tsuchiyama A (2016) Fragment shapes in impact experiments ranging from cratering to catastrophic disruption, Icarus, 264, pp. 316-330.|
|Abstract:||Laboratory impact experiments have found that impact fragments tend to be elongated. Their shapes, as defined by axes a, b and c, these being the maximum dimensions of the fragment in three mutually orthogonal planes (a≥ b≥ c), are distributed around mean values of the axial ratios b/. a~. 0.7 and c/. a~. 0.5. This corresponds to a:. b:. c in the simple proportion 2:2:1 The shape distributions of some boulders on Asteroid Eros, the small- and fast-rotating asteroids (diameter <200. m and rotation period <1 h), and asteroids in young families, are similar to those of laboratory fragments created in catastrophic disruptions. Catastrophic disruption is, however, a process that is different from impact cratering. In order to systematically investigate the shapes of fragments in the range from impact cratering to catastrophic disruption, impact experiments for basalt targets 5-15. cm in size were performed. A total of 28 impact experiments were carried out by firing a spherical nylon projectile (diameter 7.14. mm) perpendicularly into the target surface at velocities of 1.60-7.13. km/s. More than 12,700 fragments with b≥ 4 mm generated in the impact experiments were measured. We found that the mean value of c/ a in each impact decreases with decreasing impact energy per unit target mass. For instance, the mean value of c/ a in an impact cratering event is nearly 0.2, which is considerably smaller than c/ a in a catastrophic disruption (~0.5). The data presented here can provide important evidence to interpret the shapes of asteroids and boulders on asteroid surfaces, and can constrain current interpretations of asteroid formation. As an example, by applying our experimental results to the boulder shapes on Asteroid Itokawa's surface, we can infer that Itokawa's parent body must have experienced a catastrophic disruption. © 2015 The Authors.|
|Rights:||Copyright 2015 The Authors. Published by Elsevier Inc. This is an open access article under the CC BY-NC-ND license (http://creativecommons.org/licenses/by-nc-nd/4.0/).|
|1-s2.0-S0019103515004522-main.pdf||3.69 MB||Adobe PDF||View/Open|
This item is protected by original copyright
Items in the Repository are protected by copyright, with all rights reserved, unless otherwise indicated.
If you believe that any material held in STORRE infringes copyright, please contact firstname.lastname@example.org providing details and we will remove the Work from public display in STORRE and investigate your claim.