Investigation of the shocked Viñales ordinary chondrite (L6) meteorite fall – Implications for shock classification, fragmentation, and collision dynamics
Abstract
The effects of collisions on the evolution of asteroids, ranging from local fracturing to brecciation or even to catastrophic disruption, depend primarily on the encounter velocities. Here we present a refined view of the mineralogy and texture of the recent fall Viñales, an L6 ordinary chondrite meteorite. It preserves features that require at least one energetic impact, including numerous shock melt veins of variable thickness. We report the identification of two high-pressure phases, majorite and albitic jadeite, limited to just one of these shock melt veins. Viñales is a moderately shocked sample, shock stage S4, that experienced a complex and spatially variable pressure-temperature-time history with a low (but non-zero) probability of preservation of high-pressure phases.
Additional Information
I.B., S.X., and A.P. received support for this research from ESF and the Greek State (call code EDBM103). I.B. research received support from the SYNTHESYS Project (http://www.synthesys.info/ which is financed by European Community Research Infrastructure Action under the FP7 "Capacities" Program, covering travel and accommodation as well as instrument time costs at the Natural History Museum Vienna (Austria). PDA acknowledged NSF award 1725349.Additional details
- Eprint ID
- 118068
- Resolver ID
- CaltechAUTHORS:20221128-494241100.28
- European Social Fund
- EDBM103
- European Research Council (ERC)
- NSF
- EAR-1725349
- Created
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2022-12-16Created from EPrint's datestamp field
- Updated
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2022-12-16Created from EPrint's last_modified field
- Caltech groups
- Division of Geological and Planetary Sciences (GPS)