TY - JOUR
T1 - Intermineral oxygen three-isotope systematics of silicate minerals in equilibrated ordinary chondrites
AU - McDougal, David
AU - Nakashima, Daisuke
AU - Tenner, Travis J.
AU - Kita, Noriko T.
AU - Valley, John W.
AU - Noguchi, Takaaki
N1 - Funding Information:
Acknowledgments—The authors acknowledge allocation of meteorite samples from the Field Museum (Phillip Heck), the Smithsonian Institute for Natural History (Tim McCoy and Linda Welzenbach), the Muséum National d’Histoire Naturelle (Brigitte Zanda), and Dr. Naoji Sugiura. We thank Brian Hess for sample preparation, John Fournelle for assistance with electron microprobe analyses, Céline Defouilloy for assistance with SIMS analyses, Jim Kern for SIMS support, and Clark Johnson for helpful comments and discussions. The authors thank reviewers James Van Orman and Devin Schrader as well as Associate Editor Kevin Righter for comments which improved the clarity of the paper. This study is partly supported from NASA grant (NNX13AD15G, PI; Noriko Kita). WiscSIMS is partly supported by NSF-EAR (0319230, 0744079, 1053466, 1355590).
Publisher Copyright:
© The Meteoritical Society, 2017.
PY - 2017/11
Y1 - 2017/11
N2 - 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 (EOCs) 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 type 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.
AB - 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 (EOCs) 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 type 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.
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U2 - 10.1111/maps.12932
DO - 10.1111/maps.12932
M3 - Article
AN - SCOPUS:85033227162
SN - 1086-9379
VL - 52
SP - 2322
EP - 2342
JO - Meteoritics and Planetary Science
JF - Meteoritics and Planetary Science
IS - 11
ER -