 | | Journal (article/letter/editorial) | | pages 239–243, 2020 Machiite, Al2Ti3O9, a new oxide mineral from the Murchison carbonaceous chondrite:...Rossman2 1 Hawai‘i Institute of Geophysics and Planetology, University of Hawai‘i at Mānoa, Honolulu,...96822, U.S.A. Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena...Pasadena, California 91125, U.S.A. 2 Abstract Machiite (IMA 2016-067), Al2Ti3O9, is a new mineral that occurs...in a matrix of the Murchison CM2 carbonaceous chondrite. The mean chemical composition of holotype machiite |  | Ma, Chi, Krot, Alexander N., Beckett, John R., Nagashima, Kazuhide, Tschauner, Oliver, Rossman, George R., Simon, Steven B., Bischoff, Addi (2020) Warkite, Ca2Sc6Al6O20, a new mineral in carbonaceous chondrites and a key-stone phase in ultrarefractory inclusions from the solar nebula. Geochimica et Cosmochimica Acta, 277. 52-86 doi:10.1016/j.gca.2020.03.002 | Journal (article/letter/editorial) | | Bischoff g a Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena...91125, USA Hawai0 i Institute of Geophysics and Planetology, University of Hawai0 i at Manoa, Honolulu...Department of Geoscience, University of Nevada, Las Vegas, NV 89154, USA e Department of the Geophysical...The University of Chicago, Chicago, IL 60637, USA f Institute of Meteoritics, University of New Mexico,...Sc-rich ultrarefractory mineral in the rhönite group of the sapphirine supergroup. It has a P1 aenigmatite-type |  | Krot, A.N., Ma, C., Nagashima, K., Davis, A.M., Beckett, J.R., Simon, S.B., Komatsu, M., Fagan, T.J., Brenker, F., Ivanova, M.A., Bischoff, A. (2019) Mineralogy, petrography, and oxygen isotopic compositions of ultrarefractory inclusions from carbonaceous chondrites. Geochemistry, 79 (4) 125519 doi:10.1016/j.chemer.2019.07.001 | Journal (article/letter/editorial) | | MINERALOGY, PETROGRAPHY, AND OXYGEN ISOTOPIC COMPOSITIONS OF ULTRAREFRACTORY INCLUSIONS FROM CARBONACEOUS CHONDRITES...MINERALOGY, PETROGRAPHY, AND OXYGEN ISOTOPIC COMPOSITIONS OF ULTRAREFRACTORY INCLUSIONS FROM CARBONACEOUS CHONDRITES...PDF file of an article that has undergone enhancements after acceptance, such as the addition of a cover...readability, but it is not yet the definitive version of record. This version will undergo additional copyediting...are providing this version to give early visibility of the article. Please note that, during the production |  | | Book | | METEORITE MINERALOGY Meteorites are fascinating cosmic visitors. Using accessible language, this book...history of mineralogy and meteorite research, summarizes the mineralogical characteristics of the myriad...myriad varieties of meteorites, and explains the mineralogical characteristics of Solar System bodies visited...visited by spacecraft. Some of these bodies contain minerals that do not occur naturally on Earth or in...– from condensation in the expanding atmospheres of dying stars to crystallization in deep-seated magmas |  | | Journal (article/letter/editorial) | | G Model CHEMER-25420; No. of Pages 61 ARTICLE IN PRESS Chemie der Erde xxx (2017) xxx–xxx Contents...Chi Ma c a Department of Earth, Planetary, and Space Sciences, University of California, Los Angeles...90095-1567, USA Institute of Geophysics and Planetary Physics, University of California, Los Angeles,...90095-1567, USA c Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena...meteorites can be categorized as having formed by a myriad of processes that are not all mutually distinct: (1) |  | | Journal (article/letter/editorial) | | 02333. N. M. Abreu1 and K. L. Crispin2. 1Department of Chemistry, Penn State University – DuBois Campus...degrees of aqueous alteration [e.g. 1-6]. In addition, some CMs underwent substantial degrees of thermal...metamorphism of CMs resulted in low H2O and C contents, as well as partial dehydration of matrix phyllosilicates...preserved. Most prominently, CM Paris reveals some of these pre-accretionary features that therefore sheds...sheds light on the initial characteristics of the CM parent body(s) and on solar nebular processes [e |
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