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      Global Fe–O isotope correlation reveals magmatic origin of Kiruna-type apatite-iron-oxide ores

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          Abstract

          Kiruna-type apatite-iron-oxide ores are key iron sources for modern industry, yet their origin remains controversial. Diverse ore-forming processes have been discussed, comprising low-temperature hydrothermal processes versus a high-temperature origin from magma or magmatic fluids. We present an extensive set of new and combined iron and oxygen isotope data from magnetite of Kiruna-type ores from Sweden, Chile and Iran, and compare them with new global reference data from layered intrusions, active volcanic provinces, and established low-temperature and hydrothermal iron ores. We show that approximately 80% of the magnetite from the investigated Kiruna-type ores exhibit δ 56Fe and δ 18O ratios that overlap with the volcanic and plutonic reference materials (> 800 °C), whereas ~20%, mainly vein-hosted and disseminated magnetite, match the low-temperature reference samples (≤400 °C). Thus, Kiruna-type ores are dominantly magmatic in origin, but may contain late-stage hydrothermal magnetite populations that can locally overprint primary high-temperature magmatic signatures.

          Abstract

          The origin of giant Kiruna-type iron ores has been debated for nearly 100 years. This study employs extensive stable isotope data from Kiruna-type ores worldwide and magmatic and hydrothermal reference materials to show that iconic Kiruna-type ores originate primarily from ortho-magmatic processes.

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          Structural absorption by barbule microstructures of super black bird of paradise feathers

          Many studies have shown how pigments and internal nanostructures generate color in nature. External surface structures can also influence appearance, such as by causing multiple scattering of light (structural absorption) to produce a velvety, super black appearance. Here we show that feathers from five species of birds of paradise (Aves: Paradisaeidae) structurally absorb incident light to produce extremely low-reflectance, super black plumages. Directional reflectance of these feathers (0.05–0.31%) approaches that of man-made ultra-absorbent materials. SEM, nano-CT, and ray-tracing simulations show that super black feathers have titled arrays of highly modified barbules, which cause more multiple scattering, resulting in more structural absorption, than normal black feathers. Super black feathers have an extreme directional reflectance bias and appear darkest when viewed from the distal direction. We hypothesize that structurally absorbing, super black plumage evolved through sensory bias to enhance the perceived brilliance of adjacent color patches during courtship display.
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            The oxygen isotope geochemistry of igneous rocks

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              Oxygen Isotopes in Mantle and Crustal Magmas as Revealed by Single Crystal Analysis

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                Author and article information

                Contributors
                valentin.troll@geo.uu.se
                Journal
                Nat Commun
                Nat Commun
                Nature Communications
                Nature Publishing Group UK (London )
                2041-1723
                12 April 2019
                12 April 2019
                2019
                : 10
                : 1712
                Affiliations
                [1 ]ISNI 0000 0004 1936 9457, GRID grid.8993.b, Section for Mineralogy, Petrology and Tectonics, Department of Earth Sciences, , Uppsala University, ; Villavägen 16, 75236 Uppsala, Sweden
                [2 ]ISNI 0000 0004 0605 2864, GRID grid.425591.e, Swedish Museum of Natural History, Dept. of Geosciences, ; Frescativägen 40, 114 18 Stockholm, Sweden
                [3 ]ISNI 0000 0001 2179 2375, GRID grid.426025.7, Department of Mineral Resources, , Geological Survey of Sweden, ; Villavägen 18, Box 670, 75128 Uppsala, Sweden
                [4 ]Luossavaara-Kiirunavaara AB, Research & Development, FK9, 981 86 Kiruna, Sweden
                [5 ]ISNI 0000 0001 2243 211X, GRID grid.484159.5, Geological Survey of Iran, Meraj St, Azadi Sq, ; Tehran, 138783-5841 Iran
                [6 ]ISNI 0000 0001 2235 8415, GRID grid.13797.3b, Geology and Mineralogy, Åbo Akademi University, ; Domkyrkotorget 1, 20500 Turku, Finland
                [7 ]ISNI 0000 0004 1937 1151, GRID grid.7836.a, Department of Geological Sciences, , University of Cape Town, ; Rondebosch, 7701 South Africa
                [8 ]ISNI 0000 0001 0807 5670, GRID grid.5600.3, School of Earth and Ocean Sciences, Cardiff University, Park Place, ; Cardiff, CF10 3AT UK
                [9 ]ISNI 0000 0001 0744 7946, GRID grid.444703.0, National Institute of Technology Rourkela, Department of Earth & Atmospheric Sciences, NIT Rourkela, ; Odisha, 769008 India
                [10 ]Swedish Ministry of Enterprise and Innovation, Division for Business, Mäster Samuelsgatan 70, 10333 Stockholm, Sweden
                [11 ]Present Address: Indian Institute of Technology (IIT) Bombay, Department of Earth Sciences, Powai, Mumbai, 400076 India
                Article
                9244
                10.1038/s41467-019-09244-4
                6461606
                30979878
                72b652ef-ef1a-4400-a9cb-affe0a0099fa
                © The Author(s) 2019

                Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons license, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons license and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this license, visit http://creativecommons.org/licenses/by/4.0/.

                History
                : 22 March 2018
                : 22 January 2019
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