Formation mechanisms of ringwoodite: clues from the Martian meteorite Northwest Africa 8705

نویسندگان

چکیده

Abstract Ringwoodite and wadsleyite are the high-pressure polymorphs of olivine, which common in shocked meteorites. They major constituent minerals terrestrial mantle. NWA 8705, an olivine-phyric shergottite, was heavily shocked, producing shock-induced melt veins pockets associated with four occurrences ringwoodite: (1) lamellae intergrown host olivine adjacent to a pocket; (2) polycrystalline assemblages preserving shapes compositions pre-existing within vein (60 μm width); (3) rod-like grains coexisting clinopyroxene vein; (4) microlite clusters embedded silicate glass very thin (20 width). The first two ringwoodite likely formed via solid-state transformation from supported by their morphological features homogeneous (Mg# 64–62) similar 66–64). third occurrence might fractionally crystallize melt, based on its heterogeneous more FeO-enriched 76–51) than those 77–67) 66–64) this meteorite. coexistence ringwoodite, wadsleyite, suggests post-shock pressure 14–16 GPa temperature 1650–1750 °C. fourth compositional variation 72–58) crystallized at 16–18 1750–1850 presence probably due fast cooling rates and/or small pockets. In addition, higher Fa-contents (Fa 35–39 ) 8705 ordinary chondrites 16–32 makes olivine–ringwoodite prolong lower pressure.

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ژورنال

عنوان ژورنال: Earth, Planets and Space

سال: 2021

ISSN: ['1880-5981', '1343-8832']

DOI: https://doi.org/10.1186/s40623-021-01494-1