Literature DB >> 29551884

Intermineral oxygen three-isotope systematics of silicate minerals in equilibrated ordinary chondrites.

David McDougal1, Daisuke Nakashima1,2, Travis J Tenner1,3, Noriko T Kita1, John W Valley1, Takaaki Noguchi4.   

Abstract

High precision oxygen three-isotope ratios were measured for four mineral phases (olivine, low-Ca and high-Ca pyroxene, and plagioclase) in equilibrated ordinary chondrites (EOC) using a secondary ion mass spectrometer. Eleven EOCs were studied that cover all groups (H, L, LL) and petrologic types (4, 5, 6), including S1-S4 shock stages, as well as unbrecciated and brecciated meteorites. SIMS analyses of multiple minerals were made in close proximity (mostly <100 μm) from several areas in each meteorite thin section, to evaluate isotope exchange among minerals. Oxygen isotope ratios in each mineral become more homogenized as petrologic type increases with the notable exception of brecciated samples. In type 4 chondrites, oxygen isotope ratios of olivine and low-Ca pyroxene are heterogeneous in both δ18O and Δ17O, showing similar systematics to those in type 3 chondrites. In types 5 and 6 chondrites, oxygen isotope ratios of the four mineral phases plot along mass dependent fractionation lines that are consistent with the bulk average Δ17O of each chondrite group. The δ18O of three minerals, low-Ca and high-Ca pyroxene and plagioclase, are consistent with equilibrium fractionation at temperatures of 700-1000°C. In most cases the δ18O values of olivine are higher than those expected from pyroxene and plagioclase, suggesting partial retention of premetamorphic values due to slower oxygen isotope diffusion in olivine than pyroxene during thermal metamorphism in ordinary chondrite parent bodies.

Entities:  

Keywords:  Oxygen isotope ratios; SIMS; equilibrated ordinary chondrites

Year:  2017        PMID: 29551884      PMCID: PMC5849465          DOI: 10.1111/maps.12932

Source DB:  PubMed          Journal:  Meteorit Planet Sci        ISSN: 1086-9379            Impact factor:   2.487


  4 in total

1.  Structure and thermal history of the H-chondrite parent asteroid revealed by thermochronometry.

Authors:  Mario Trieloff; Elmar K Jessberger; Ingrid Herrwerth; Jens Hopp; Christine Fiéni; Marianne Ghélis; Michèle Bourot-Denise; Paul Pellas
Journal:  Nature       Date:  2003-04-03       Impact factor: 49.962

2.  Fast delivery of meteorites to Earth after a major asteroid collision.

Authors:  Philipp R Heck; Birger Schmitz; Heinrich Baur; Alex N Halliday; Rainer Wieler
Journal:  Nature       Date:  2004-07-15       Impact factor: 49.962

3.  The oxygen isotopic composition of the Sun inferred from captured solar wind.

Authors:  K D McKeegan; A P A Kallio; V S Heber; G Jarzebinski; P H Mao; C D Coath; T Kunihiro; R C Wiens; J E Nordholt; R W Moses; D B Reisenfeld; A J G Jurewicz; D S Burnett
Journal:  Science       Date:  2011-06-24       Impact factor: 47.728

4.  Remnants of the early solar system water enriched in heavy oxygen isotopes.

Authors:  Naoya Sakamoto; Yusuke Seto; Shoichi Itoh; Kiyoshi Kuramoto; Kiyoshi Fujino; Kazuhide Nagashima; Alexander N Krot; Hisayoshi Yurimoto
Journal:  Science       Date:  2007-06-14       Impact factor: 47.728

  4 in total

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