Avdellidou, Chrysoula, Price, M. C., Delbo, M., Cole, M. J. (2016) Survival of the impactor during hypervelocity collisions – II. An analogue for high-porosity targets. Monthly Notices of the Royal Astronomical Society, 464 (1). pp. 734-738. ISSN 0035-8711. (doi:10.1093/mnras/stw2381) (The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided) (KAR id:61421)
| The full text of this publication is not currently available from this repository. You may be able to access a copy if URLs are provided. | |
| Official URL: https://doi.org/10.1093/mnras/stw2381 |
Abstract
We investigated how a target's porosity affects the outcome of a collision, with respect to the impactor's fate. Laboratory impact experiments using peridot projectiles were performed at a speed range between 0.3 and 3.0 km s?1, on to high-porosity water-ice (40 per cent) and fine-grained calcium carbonate (70 per cent) targets. We report that the amount of implanted material in the target body increases with increasing target's porosity, while the size frequency distribution of the projectile's ejecta fragments becomes steeper. A supplementary Raman study showed no sign of change of the Raman spectra of the recovered olivine projectile fragments indicate minimal physical change.
| Item Type: | Article |
|---|---|
| DOI/Identification number: | 10.1093/mnras/stw2381 |
| Uncontrolled keywords: | techniques: image processing, minor planets, asteroids: general |
| Divisions: | Divisions > Division of Natural Sciences > Physics and Astronomy |
| Depositing User: | Mark Price |
| Date Deposited: | 21 Apr 2017 08:40 UTC |
| Last Modified: | 05 Nov 2024 10:55 UTC |
| Resource URI: | https://kar.kent.ac.uk/id/eprint/61421 (The current URI for this page, for reference purposes) |
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