¹Y Ellinger,¹M Lattelais,¹F Pauzat,²J-C Guillemin,³B Zanda
Monthly Notices of the Royal Astronomical Society 502, 4064–4073 Link to Article [https://doi.org/10.1093/mnras/stab217]
¹Sorbonne Université, CNRS – UMR7616, LCT, 4 Place Jussieu, F-75005 Paris, France
²Univ Rennes, Ecole Nationale Supérieure de Chimie de Rennes, CNRS, ISCR UMR6226, F-35000 Rennes, France
³Sorbonne Université, CNRS – UMR7202, MNHN, 61 rue Buffon, F-75005 Paris, France

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^1,2,3Jarmo Moilanen,^1,2,3,4Maria Gritsevich,³Esko Lyytinen
Monthly Notices of the Royal Astronomical Society 503, 3337–3350 Link to Article [https://doi.org/10.1093/mnras/stab586]
¹Finnish Geospatial Research Institute (FGI), Geodeetinrinne 2, FI-02430 Masala, Finland
²University of Helsinki, Faculty of Science, Gustaf Hällsrömin katu 2, FI-00014 Helsinki, Finland
³Finnish Fireball Network, Ursa Astronomical Association, Kopernikuksentie 1, FI-00130 Helsinki, Finland
⁴Institute of Physics and Technology, Ural Federal University, Ekaterinburg 620002, Russia

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¹Sujoy Ghosh¹Kishan Tiwari,²Masaaki Miyahara,³Arno Rohrbach,³Christian Vollmer,⁴Vincenzo Stagno,⁵Eiji Ohtani,⁶Dwijesh Ray
Proceedings of the National Academy of the United States of America (in press) Link to Article [https://doi.org/10.1073/pnas.2108736118]
¹Department of Geology and Geophysics, Indian Institute of Technology Kharagpur, Kharagpur 721302, India;
²Graduate School of Advanced Science and Engineering, Hiroshima University, Hiroshima 739-8526, Japan;
³Institut für Mineralogie, Westfälische Wilhelms-Universität Münster, 48149 Münster, Germany;
⁴Department of Earth Sciences, Sapienza University of Rome, Rome 00185, Italy;
⁵Department of Earth and Planetary Materials Science, Graduate School of Sciences, Tohoku University, Sendai 980-8578, Japan;
⁶Planetary Sciences Division, Physical Research Laboratory, Ahmedabad 380009, India

Bridgmanite, the most abundant mineral of the Earth’s lower mantle, has been reported in only a few shocked chondritic meteorites; however, the compositions of these instances differ from that expected in the terrestrial bridgmanite. Here, we report the first natural occurrence of Fe-bearing aluminous bridgmanite in shock-induced melt veins within the Katol L6 chondrite with a composition that closely matches those synthesized in high-pressure and temperature experiments over the last three decades. The Katol bridgmanite coexists with majorite and metal-sulfide intergrowths. We found that the natural Fe-bearing aluminous bridgmanite in the Katol L6 chondrite has a significantly higher Fe³⁺/ΣFe ratio (0.69 ± 0.08) than coexisting majorite (0.37 ± 0.10), which agrees with experimental studies. The Katol bridgmanite is arguably the closest natural analog for the bridgmanite composition expected to be present in the Earth’s lower mantle. Textural observations and comparison with laboratory experiments suggest that the Katol bridgmanite formed at pressures of ∼23 to 25 gigapascals directly from the chondritic melt generated by the shock event. Thus, the Katol L6 sample may also serve as a unique analog for crystallization of bridgmanite during the final stages of magma ocean crystallization during Earth’s formation.