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Published on: November 21, 2013
Rock fluidization during peak-ring formation of large impact structures.
Ulrich Riller1, Michael H Poelchau2, Auriol S P Rae3
1Institut für Geologie, Universität Hamburg, Hamburg, Germany. ulrich.riller@uni-hamburg.de.
Meteorite impacts cause rocks to drastically weaken, flow, and then regain strength to form impact rings. This study reveals acoustic fluidization as a key process in cratering mechanics.
Area of Science:
- Planetary Science
- Geology
- Impact Cratering
Background:
- Terrestrial impact structures exhibit prominent topographic rings formed by uplifted crustal rocks.
- The rapid deformation and subsequent strength recovery of these rocks during cratering remain poorly understood.
Purpose of the Study:
- To investigate the mechanisms of rock deformation responsible for the formation of impact crater rings.
- To elucidate the processes of catastrophic weakening and strength recovery in target rocks during large impacts.
Main Methods:
- Analysis of core samples from the Chicxulub impact structure.
- Examination of brittle and viscous deformation within peak-ring rocks.
Main Results:
- Observed catastrophic rock weakening followed by strength increase during cratering.
- Evidence suggests acoustic fluidization as the dominant initial cratering process.
- Subsequent crater formation involved increasingly localized faulting.
Conclusions:
- Acoustic fluidization explains the initial rapid flow and large-scale deformation of target rocks.
- The transition from fluidization to localized faulting explains the formation and sustainment of topographic rings in impact structures.
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