CHONDRITES: MAGNETIC SUSCEPTIBILITY AND TYPE II CHONDRULE OLIVINE Cr2O3 CONTENTS AND THEIR IMPLICATIONS FOR PAIRING. K. Righter, H. Busemann, L. M. Eckart, C. Alexander, J. Schutt, R. Harvey, and J. Karner, Mailcode XI2, NASA Johnson Space Center, 2101 NASA Pkwy, Houston, TX, 77058, USA, ETH Zürich, Inst. Geochem. Petrol, Clausiusstrasse 25, 8092 Zürich, Switzerland; Earth and Planets Laboratory, Carnegie Institution for Science, 5241 Broad Branch Road, NW, Washington, DC 20015-1305; 4 EEPS, Case Western Reserve University, Cleveland, OH 44106; Geology & Geophysics, University of Utah, Salt Lake City UT 84112.

SURVEY OF DOMINION RANGE (DOM) AND MILLER RANGE (MIL) CO3 CARBONACEOUS CHONDRITES: MAGNETIC SUSCEPTIBILITY AND TYPE II CHONDRULE OLIVINE Cr2O3 CONTENTS AND THEIR IMPLICATIONS FOR PAIRING

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SURVEY OF DOMINION RANGE (DOM) AND MILLER RANGE (MIL) CO3 CARBONACEOUS CHONDRITES: MAGNETIC SUSCEPTIBILITY AND TYPE II CHONDRULE OLIVINE Cr2O3 CONTENTS AND THEIR IMPLICATIONS FOR PAIRING