Repository logo
  • English
  • Italiano
Log In
New user? Click here to register.Have you forgotten your password?
  1. Home
  2. Affiliation
  3. INGV
  4. Article published / in press
  5. Coseismic recrystallization during shallow earthquake slip
 
  • Details

Coseismic recrystallization during shallow earthquake slip

Author(s)
Smith, S. A. F.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia  
Di Toro, G.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia  
Kim, S.  
Department of Earth and Environmental Sciences, Korea University, Seoul 136-701, Republic of Korea  
Ree, J.-H.  
Department of Earth and Environmental Sciences, Korea University, Seoul 136-701, Republic of Korea  
Nielsen, S. B.  
Istituto Nazionale di Geofisica e Vulcanologia, Sezione Roma1, Roma, Italia  
Billi, A.  
Consiglio Nazionale delle Ricerche, Istituto di Geologia Ambientale e Geoingegneria, c.o. Dipartimento Scienze della Terra, Sapienza Università di Roma, 00185 Rome, Italy  
Spiess, R.  
Dipartimento delle Scienze della Terra, Università degli Studi di Padova, Via G. Gradenigo 6, 35131 Padua, Italy  
Language
English
Obiettivo Specifico
4T. Fisica dei terremoti e scenari cosismici
Status
Published
JCR Journal
JCR Journal
Peer review journal
Yes
Journal
Geology (Geological Society of America)  
Issue/vol(year)
1/41(2013)
ISSN
0091-7613
Electronic ISSN
1943-2682
Publisher
Geological Society of America
Pages (printed)
63-66
Date Issued
October 2013
DOI
10.1130/G33588.1
URI
https://www.earth-prints.org/handle/2122/9312
Subjects
04. Solid Earth::04.01. Earth Interior::04.01.04. Mineral physics and properties of rocks  
04. Solid Earth::04.04. Geology::04.04.06. Rheology, friction, and structure of fault zones  
04. Solid Earth::04.04. Geology::04.04.09. Structural geology  
04. Solid Earth::04.07. Tectonophysics::04.07.07. Tectonics  
Subjects

Rock mechanics

shallow earthquales

Abstract
Solidified frictional melts, or pseudotachylytes, remain the only unambiguous indicator of seismic slip in the geological record. However, pseudotachylytes form at >5 km depth, and there are many rock types in which they do not form at all. We performed low- to high-velocity rock friction experiments designed to impose realistic coseismic slip pulses on calcite fault gouges, and report that localized dynamic recrystallization may be an easy-to-recognize microstructural indicator of seismic slip in shallow, otherwise brittle fault zones. Calcite gouges with starting grain size <250 μm were confined up to 26 MPa normal stress using a purpose-built sample holder. Slip velocities were between 0.01 and 3.4 m s−1, and total displacements between 1 and 4 m. At coseismic slip velocities ≥0.1 m s−1, the gouges were cut by reflective principal slip surfaces lined by polygonal grains <1 μm in size. The principal slip surfaces were flanked by <300 μm thick layers of dynamically recrystallized calcite (grain size 1–10 μm) containing well-defined shape- and crystallographic-preferred orientations. Dynamic recrystallization was accompanied by fault weakening and thermal decomposition of calcite to CO2 + CaO. The recrystallized calcite aggregates resemble those found along the principal slip surface of the Garam thrust, South Korea, exhumed from <5 km depth. We suggest that intense frictional heating along the experimental and natural principal slip surfaces resulted in localized dynamic recrystallization, a microstructure that may be diagnostic of seismic slip in the shallow crust.
Type
article
File(s)
Loading...
Thumbnail Image
Name

GEology-2013-Smith.pdf

Size

1.46 MB

Format

Adobe PDF

Checksum (MD5)

2566345131c65d160719bfe58451007e

rome library|catania library|milano library|napoli library|pisa library|palermo library
Explore By
  • Research Outputs
  • Researchers
  • Organizations
Info
  • Earth-Prints Open Archive Brochure
  • Earth-Prints Archive Policy
  • Why should you use Earth-prints?
Earth-prints working group
⚬Anna Grazia Chiodetti (Project Leader)
⚬Gabriele Ferrara (Technical and Editorial Assistant)
⚬Massimiliano Cascone
⚬Francesca Leone
⚬Salvatore Barba
⚬Emmanuel Baroux
⚬Roberto Basili
⚬Paolo Marco De Martini

Built with DSpace-CRIS software - Extension maintained and optimized by 4Science

  • Privacy policy
  • End User Agreement
  • Send Feedback