Petrography and shock-related remagnetization of pyrrhotite in drill cores from the Bosumtwi Impact Crater Drilling Project, Ghana
dc.contributor.author | Kontny, A. | |
dc.contributor.author | Elbra, T. | |
dc.contributor.author | Just, J. | |
dc.contributor.author | Pesonen, L. J. | |
dc.contributor.author | Schleicher, A. M. | |
dc.contributor.author | Zolk, J. | |
dc.date.accessioned | 2021-02-12T22:54:25Z | |
dc.date.available | 2021-02-12T22:54:25Z | |
dc.date.issued | 2007-01-01 | |
dc.identifier.citation | Kontny, A., Elbra, T., Just, J., Pesonen, L. J., Schleicher, A. M., & Zolk, J. (2007). Petrography and shock‐related remagnetization of pyrrhotite in drill cores from the Bosumtwi Impact Crater Drilling Project, Ghana. Meteoritics & Planetary Science, 42(4‐5), 811-827. | |
dc.identifier.issn | 1945-5100 | |
dc.identifier.doi | 10.1111/j.1945-5100.2007.tb01077.x | |
dc.identifier.uri | http://hdl.handle.net/10150/656709 | |
dc.description.abstract | Rock magnetic and magnetic mineralogy data are presented from the International Continental Scientific Drilling Program (ICDP) drill cores LB-07A and LB-08A of the Bosumtwi impact structure in order to understand the magnetic behavior of impact and target lithologies and their impact-related remagnetization mechanism. Basic data for the interpretation of the magnetic anomaly patterns and the magnetic borehole measurements as well as for new magnetic modeling are provided. Magnetic susceptibility (150-500 10^)-6) SI) and natural remanent magnetization (10^(-3)-10^(-1) A/m) are generally weak, but locally higher values up to 10.6 x 10^(-3) SI and 43 A/m occur. Sixty-three percent of the investigated rock specimens show Q values above 1 indicating that remanence clearly dominates over induced magnetization, which is a typical feature of impact structures. Ferrimagnetic pyrrhotite is the main magnetite phase, which occurs besides minor magnetite and a magnetic phase with a Curie temperature between 330 and 350 degrees C, interpreted as anomalous pyrrhotite. Coercive forces are between 20 and 40 mT. Brecciation and fracturing of pyrrhotite is a common feature confirming its pre-impact origin. Grain sizes of pyrrhotite show a large variation but the numerous stress-induced nanostructures observable by transmission electron microscopy (TEM) are assumed to behave as single-domain grains. We suggest that the drilled rocks lost their pre-shock remanence memory during the shock event and acquired a new, stable remanence during shock-induced grain size reduction. The observed brittle microstructures indicate temperatures not higher than 250 degrees C, which is below the Curie temperature of ferrimagnetic pyrrhotite (310 degrees C). | |
dc.language.iso | en | |
dc.publisher | The Meteoritical Society | |
dc.relation.url | https://meteoritical.org/ | |
dc.rights | Copyright © The Meteoritical Society | |
dc.rights.uri | http://rightsstatements.org/vocab/InC/1.0/ | |
dc.subject | magnetic properties | |
dc.subject | remagnetization mechanism | |
dc.subject | Bosumtwi Ghana impact crater | |
dc.subject | Pyrrhotite | |
dc.title | Petrography and shock-related remagnetization of pyrrhotite in drill cores from the Bosumtwi Impact Crater Drilling Project, Ghana | |
dc.type | Article | |
dc.type | text | |
dc.identifier.journal | Meteoritics & Planetary Science | |
dc.description.collectioninformation | The Meteoritics & Planetary Science archives are made available by the Meteoritical Society and the University of Arizona Libraries. Contact lbry-journals@email.arizona.edu for further information. | |
dc.eprint.version | Final published version | |
dc.description.admin-note | Migrated from OJS platform February 2021 | |
dc.source.volume | 42 | |
dc.source.issue | 4-5 | |
dc.source.beginpage | 811 | |
dc.source.endpage | 827 | |
refterms.dateFOA | 2021-02-12T22:54:25Z |