EconPapers    
Economics at your fingertips  
 

Rock fluidization during peak-ring formation of large impact structures

Ulrich Riller (), Michael H. Poelchau, Auriol S. P. Rae, Felix M. Schulte, Gareth S. Collins, H. Jay Melosh, Richard A. F. Grieve, Joanna V. Morgan, Sean P. S. Gulick, Johanna Lofi, Abdoulaye Diaw, Naoma McCall and David A. Kring
Additional contact information
Ulrich Riller: Institut für Geologie, Universität Hamburg
Michael H. Poelchau: Universität Freiburg
Auriol S. P. Rae: Imperial College London
Felix M. Schulte: Institut für Geologie, Universität Hamburg
Gareth S. Collins: Imperial College London
H. Jay Melosh: Purdue University
Richard A. F. Grieve: Western University
Joanna V. Morgan: Imperial College London
Sean P. S. Gulick: University of Texas
Johanna Lofi: Géosciences Montpellier, CNRS, Université de Montpellier
Abdoulaye Diaw: Géosciences Montpellier, CNRS, Université de Montpellier
Naoma McCall: University of Texas
David A. Kring: Universities Space Research Association, Lunar and Planetary Institute

Nature, 2018, vol. 562, issue 7728, 511-518

Abstract: Abstract Large meteorite impact structures on the terrestrial bodies of the Solar System contain pronounced topographic rings, which emerged from uplifted target (crustal) rocks within minutes of impact. To flow rapidly over large distances, these target rocks must have weakened drastically, but they subsequently regained sufficient strength to build and sustain topographic rings. The mechanisms of rock deformation that accomplish such extreme change in mechanical behaviour during cratering are largely unknown and have been debated for decades. Recent drilling of the approximately 200-km-diameter Chicxulub impact structure in Mexico has produced a record of brittle and viscous deformation within its peak-ring rocks. Here we show how catastrophic rock weakening upon impact is followed by an increase in rock strength that culminated in the formation of the peak ring during cratering. The observations point to quasi-continuous rock flow and hence acoustic fluidization as the dominant physical process controlling initial cratering, followed by increasingly localized faulting.

Keywords: Peak-ring Formation; Target Rocks; Acoustic Fluidization; Chicxulub; Cataclasite Zones (search for similar items in EconPapers)
Date: 2018
References: Add references at CitEc
Citations:

Downloads: (external link)
https://www.nature.com/articles/s41586-018-0607-z Abstract (text/html)
Access to the full text of the articles in this series is restricted.

Related works:
This item may be available elsewhere in EconPapers: Search for items with the same title.

Export reference: BibTeX RIS (EndNote, ProCite, RefMan) HTML/Text

Persistent link: https://EconPapers.repec.org/RePEc:nat:nature:v:562:y:2018:i:7728:d:10.1038_s41586-018-0607-z

Ordering information: This journal article can be ordered from
https://www.nature.com/

DOI: 10.1038/s41586-018-0607-z

Access Statistics for this article

Nature is currently edited by Magdalena Skipper

More articles in Nature from Nature
Bibliographic data for series maintained by Sonal Shukla () and Springer Nature Abstracting and Indexing ().

 
Page updated 2025-03-19
Handle: RePEc:nat:nature:v:562:y:2018:i:7728:d:10.1038_s41586-018-0607-z