Ultrafast olivine-ringwoodite transformation during shock compression
- PMID: 34262045
- PMCID: PMC8280208
- DOI: 10.1038/s41467-021-24633-4
Ultrafast olivine-ringwoodite transformation during shock compression
Abstract
Meteorites from interplanetary space often include high-pressure polymorphs of their constituent minerals, which provide records of past hypervelocity collisions. These collisions were expected to occur between kilometre-sized asteroids, generating transient high-pressure states lasting for several seconds to facilitate mineral transformations across the relevant phase boundaries. However, their mechanisms in such a short timescale were never experimentally evaluated and remained speculative. Here, we show a nanosecond transformation mechanism yielding ringwoodite, which is the most typical high-pressure mineral in meteorites. An olivine crystal was shock-compressed by a focused high-power laser pulse, and the transformation was time-resolved by femtosecond diffractometry using an X-ray free electron laser. Our results show the formation of ringwoodite through a faster, diffusionless process, suggesting that ringwoodite can form from collisions between much smaller bodies, such as metre to submetre-sized asteroids, at common relative velocities. Even nominally unshocked meteorites could therefore contain signatures of high-pressure states from past collisions.
© 2021. The Author(s).
Conflict of interest statement
The authors declare no competing interests.
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References
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- Brearley, A. J. & Jones, R. H. Chondritic meteorites in Planetary Materials (Papike, J. J. ed.) 3-001-3-398 (Mineralogical Society of America, Chantilly, VA, 1998).
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