Please use this identifier to cite or link to this item:
Appears in Collections:Biological and Environmental Sciences Journal Articles
Peer Review Status: Refereed
Title: Properties and distribution of paired candidate stony meteorites at Meridiani Planum, Mars
Authors: Schröder, Christian
Herkenhoff, Kenneth E
Farrand, William H
Chappelow, John H
Wang, Wei
Nittler, Larry R
Ashley, James W
Fleischer, Iris
Gellert, Ralf
Golombek, Matthew
Johnson, Jeffrey R
Klingelhoefer, Goestar
Li, Ron
Morris, Richard Van
Squyres, Steven W
Contact Email:
Keywords: impact
meteorite accumulation
Issue Date: Jul-2010
Publisher: American Geophysical Union
Citation: Schröder C, Herkenhoff KE, Farrand WH, Chappelow JH, Wang W, Nittler LR, Ashley JW, Fleischer I, Gellert R, Golombek M, Johnson JR, Klingelhoefer G, Li R, Morris RV & Squyres SW (2010) Properties and distribution of paired candidate stony meteorites at Meridiani Planum, Mars, Journal of Geophysical Research: Planets, 115 (E7), Art. No.: E00F09.
Abstract: The Mars Exploration Rover Opportunity investigated four rocks, informally dubbed Barberton, Santa Catarina, Santorini, and Kasos, that are possible stony meteorites. Their chemical and mineralogical composition is similar to the howardite, eucrite, and diogenite group but with additional metal, similar to mesosiderite silicate clasts. Because of their virtually identical composition and because they appear to represent a relatively rare group of meteorites, they are probably paired. The four rocks were investigated serendipitously several kilometers apart, suggesting that Opportunity is driving across a larger population of similar rock fragments, maybe a meteorite strewn field. Small amounts of ferric Fe are a result of weathering. We did not observe evidence for fusion crusts. Four iron meteorites were found across the same area. Although mesosiderites are stony irons, a genetic link to these irons is unlikely. The stony meteorites probably fell later than the irons. The current atmosphere is sufficiently dense to land such meteorites at shallow entry angles, and it would disperse fragments over several kilometers upon atmospheric breakup. Alternatively, dispersion by spallation from an impacting meteoroid may have occurred. Santa Catarina and a large accumulation of similar rocks were found at the rim of Victoria crater. It is possible that they are associated with the impactor that created Victoria crater, but our limited knowledge about their distribution cannot exclude mere coincidence.
Type: Journal Article
DOI Link:
Rights: Copyright 2010 by the American Geophysical Union. AGU allows authors to deposit their journal articles if the version is the final published citable version of record, the AGU copyright statement is clearly visible on the posting, and the posting is made 6 months after official publication by the AGU.
Affiliation: Biological and Environmental Sciences
U.S. Geological Survey
Space Science Institute
Meteorifics, Alaska, USA
Ohio State University
Carnegie Institution for Science
Arizona State University
Johannes Gutenberg University of Mainz
University of Guelph
California Institute of Technology
U.S. Geological Survey
Johannes Gutenberg University of Mainz
Ohio State University
National Aeronautics and Space Administration (NASA)
Cornell University

Files in This Item:
File Description SizeFormat 
Schroeder2010_properties_and_distribution_of_paired_candidate_stony_meteorites.pdf7.28 MBAdobe PDFView/Open

This item is protected by original copyright

Items in the Repository are protected by copyright, with all rights reserved, unless otherwise indicated.

If you believe that any material held in STORRE infringes copyright, please contact providing details and we will remove the Work from public display in STORRE and investigate your claim.