New high-pressure Fe-Ti oxide minerals in the Shergotty Martian meteorite: Feiite, Fe2+2(Fe2+Ti4+)O5, liuite, FeTiO3, and tschaunerite, (Fe2+)(Fe2+Ti4+)O4

IF 2.2 4区 地球科学 Q2 GEOCHEMISTRY & GEOPHYSICS
Chi Ma, Oliver Tschauner, John R. Beckett, Vitali B. Prakapenka
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引用次数: 0

Abstract

High-pressure oxides like perovskite-type FeTiO3, CaTi2O4-type Fe2TiO4, and ferrous-ferric oxides that form polysomes between wüstite and CaFe2O4-type Fe3O4 are potential carriers of Fe, Ti, and other transition metals in the mantle and may play an important role in the redox budget of the deep Earth. Here, we report the occurrence of three of these phases as the new minerals: feiite (Sr2Tl2O5-type Fe2+2(Fe2+Ti4+)O5), liuite (FeTiO3 with a GdFeO3-type perovskite structure), and tschaunerite (CaTi2O4-type (Fe2+)(Fe2+Ti4+)O4), along with wangdaodeite (LiNbO3-type FeTiO3) in a transformed ulvöspinel clast entrained in a shock melt pocket in the Shergotty Martian meteorite. We show that reaction between the shocked ulvöspinel precursor and melt occurred at pressures between 20 and 25 GPa. The high-pressure Fe-, Ti-minerals lost Fe and O to the surrounding shock melt in exchange for Si, Mg, and Ca. Concentrations of Si and Mg in all of these clast phases and of Na in liuite are significant. They substantiate chemical interaction of the clast with melt during the shock event and highlight potential elemental distributions in complex Fe- and Ti-rich lithologies at pressures of the deep transition zone to shallow lower mantle.

Shergotty火星陨石中新的高压Fe-Ti氧化物矿物:feite, Fe2+2(Fe2+Ti4+)O5, liite, FeTiO3, tschaunerite, (Fe2+)(Fe2+Ti4+)O4
高压氧化物如钙钛矿型FeTiO3, cati2o4型Fe2TiO4,以及在w stite和cafe2o4型Fe3O4之间形成多体的铁-铁氧化物是地幔中Fe, Ti等过渡金属的潜在载体,可能在地球深部的氧化还原收支中发挥重要作用。本文报道了其中三种相的新矿物:飞石(sr2tl2o5型Fe2+2(Fe2+Ti4+)O5)、柳石(具有gdfeo3型钙钛矿结构的FeTiO3)、闪辉石(cati2o4型(Fe2+)(Fe2+Ti4+)O4),以及王道德石(linbo3型FeTiO3),在Shergotty火星陨石的冲击熔体袋中携带的转化ulvöspinel碎屑中出现。结果表明,冲击ulvöspinel前驱体与熔体之间的反应发生在20至25 GPa的压力之间。高压Fe-、ti -矿物将Fe和O转移到周围的激波熔体中,以换取Si、Mg和Ca。所有这些碎屑相中Si和Mg的浓度以及流岩中Na的浓度都是显著的。它们证实了在冲击事件中碎屑与熔体的化学相互作用,并突出了深部过渡带至下地幔浅层压力下复杂富铁和富钛岩性中潜在的元素分布。
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来源期刊
Meteoritics & Planetary Science
Meteoritics & Planetary Science 地学天文-地球化学与地球物理
CiteScore
3.90
自引率
31.80%
发文量
121
审稿时长
3 months
期刊介绍: First issued in 1953, the journal publishes research articles describing the latest results of new studies, invited reviews of major topics in planetary science, editorials on issues of current interest in the field, and book reviews. The publications are original, not considered for publication elsewhere, and undergo peer-review. The topics include the origin and history of the solar system, planets and natural satellites, interplanetary dust and interstellar medium, lunar samples, meteors, and meteorites, asteroids, comets, craters, and tektites. Our authors and editors are professional scientists representing numerous disciplines, including astronomy, astrophysics, physics, geophysics, chemistry, isotope geochemistry, mineralogy, earth science, geology, and biology. MAPS has subscribers in over 40 countries. Fifty percent of MAPS'' readers are based outside the USA. The journal is available in hard copy and online.
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