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      High‐pressure minerals in shocked meteorites

      1 , 2
      Meteoritics & Planetary Science
      Wiley

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          Shock metamorphism of ordinary chondrites

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            Hydrous mantle transition zone indicated by ringwoodite included within diamond.

            The ultimate origin of water in the Earth's hydrosphere is in the deep Earth--the mantle. Theory and experiments have shown that although the water storage capacity of olivine-dominated shallow mantle is limited, the Earth's transition zone, at depths between 410 and 660 kilometres, could be a major repository for water, owing to the ability of the higher-pressure polymorphs of olivine--wadsleyite and ringwoodite--to host enough water to comprise up to around 2.5 per cent of their weight. A hydrous transition zone may have a key role in terrestrial magmatism and plate tectonics, yet despite experimental demonstration of the water-bearing capacity of these phases, geophysical probes such as electrical conductivity have provided conflicting results, and the issue of whether the transition zone contains abundant water remains highly controversial. Here we report X-ray diffraction, Raman and infrared spectroscopic data that provide, to our knowledge, the first evidence for the terrestrial occurrence of any higher-pressure polymorph of olivine: we find ringwoodite included in a diamond from Juína, Brazil. The water-rich nature of this inclusion, indicated by infrared absorption, along with the preservation of the ringwoodite, is direct evidence that, at least locally, the transition zone is hydrous, to about 1 weight per cent. The finding also indicates that some kimberlites must have their primary sources in this deep mantle region.
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              Chelyabinsk airburst, damage assessment, meteorite recovery, and characterization.

              The asteroid impact near the Russian city of Chelyabinsk on 15 February 2013 was the largest airburst on Earth since the 1908 Tunguska event, causing a natural disaster in an area with a population exceeding one million. Because it occurred in an era with modern consumer electronics, field sensors, and laboratory techniques, unprecedented measurements were made of the impact event and the meteoroid that caused it. Here, we document the account of what happened, as understood now, using comprehensive data obtained from astronomy, planetary science, geophysics, meteorology, meteoritics, and cosmochemistry and from social science surveys. A good understanding of the Chelyabinsk incident provides an opportunity to calibrate the event, with implications for the study of near-Earth objects and developing hazard mitigation strategies for planetary protection.
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                Author and article information

                Contributors
                (View ORCID Profile)
                (View ORCID Profile)
                Journal
                Meteoritics & Planetary Science
                Meteorit Planet Sci
                Wiley
                1086-9379
                1945-5100
                July 02 2017
                September 2017
                July 02 2017
                September 2017
                : 52
                : 9
                : 2017-2039
                Affiliations
                [1 ]Kochi Institute for Core Sample Research Japan Agency for Marine‐Earth Science and Technology Nankoku Kochi 783‐8502 Japan
                [2 ]Department of Earth and Planetary Systems Science Graduate School of Science Hiroshima University Higashi‐Hiroshima Hiroshima 739‐8526 Japan
                Article
                10.1111/maps.12902
                5804c6f3-32e9-48e4-bfc7-bcddabae76ec
                © 2017

                http://onlinelibrary.wiley.com/termsAndConditions#vor

                http://doi.wiley.com/10.1002/tdm_license_1.1

                History

                Quantitative & Systems biology,Biophysics
                Quantitative & Systems biology, Biophysics

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