首页> 外文期刊>Mineralogical Magazine >New minerals tsangpoite Ca-5(PO4)(2)(SiO4) and matyhite Ca-9(Ca-0.5 square(0.5))Fe(PO4)(7) from the D'Orbigny angrite
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New minerals tsangpoite Ca-5(PO4)(2)(SiO4) and matyhite Ca-9(Ca-0.5 square(0.5))Fe(PO4)(7) from the D'Orbigny angrite

机译:新型矿物质Tsangpoite Ca-5(PO4)(2)(SiO 4)和Matyhite Ca-9(Ca-0.5平方(0.5))Fe(PO4)(7)来自D'Orbigny angrite

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摘要

Tsangpoite, ideally Ca-5(PO4)(2)(SiO4), the hexagonal polymorph of silicocarnotite, and matyhite, ideally Ca-9(Ca-0.5 square(0.5))Fe(PO4)(7), the Fe-analogue of Ca-merrillite, were identified from the D'Orbigny angrite meteorite by electron probe microanalysis, electron microscopy and micro-Raman spectroscopy. On the basis of electron diffraction, the symmetry of tsangpoite was shown to be hexagonal, P6(3)/m or P6(3), with a = 9.489(4) angstrom, c = 6.991(6) angstrom, V = 545.1(6) angstrom(3) and Z = 2 for 12 oxygen atoms per formula unit, and that of matyhite was shown to be trigonal, R3c, with a = 10.456 (7) angstrom, c = 37.408(34) angstrom, V = 3541.6 (4.8) angstrom(3) and Z = 6 for 28 oxygen atoms per formula unit. On the basis of their constant association with the grain-boundary assemblage: Fe sulfide + ulvospinel + Al-Ti-bearing hedenbergite + fayalite-kirschsteinite intergrowth, the formation of tsangpoite and matyhite, along with kuratite (the Fe-analogue of rhonite), can be readily rationalised as crystallisation from residue magmas at the final stage of the D'Orbigny meteorite formation. Alternatively, the close petrographic relations between tsangpoite/matyhite and the resorbed Fe sulfide rimmed by fayalite + kirschsteinite symplectite, such as the nucleation of tsangpoite in association with magnetite +/- other phases within Fe sulfide and the common outward growth of needle-like tsangpoite or plate-like matyhite from the fayalite-kirschsteinite symplectic rim of Fe sulfide into hedenbergite, infer that these new minerals and the grain-boundary assemblage might represent metasomatic products resulting from reactions between an intruding metasomatic agent and the porous olivine-plagioclase plate + fayalite-kirschsteinite overgrowth + augite + Fe sulfide aggregates. Still further thermochemical and kinetics evidence is required to clarify the exact formation mechanisms/conditions of the euhedral tsangpoite, matyhite and kuratite at the grain boundary of the D'Orbigny angrite.
机译:Tsangpoite,理想情况下,CA-5(PO4)(2)(SiO 4),硅藻土的六角形多晶型物,和麦提钛矿,理想情况下Ca-9(Ca-0.5平方(0.5))Fe(PO4)(7),Fe样品通过电子探针微透析,电子显微镜和微拉曼光谱从D'Orbigny Angrite陨石鉴定了Ca-Merriillite。基于电子衍射,Tsangpoite的对称性显示为六边形,p6(3)/ m或p6(3),α= 9.489(4)埃,C = 6.991(6)埃,V = 545.1( 6)每种配方单元的12个氧原子的埃赫斯特罗姆(3)和Z = 2,并且麦克酸盐的抗麦克酸术是三角形的R3C,A = 10.456(7)埃,C = 37.408(34)埃,V = 3541.6 (4.8)埃赫斯特罗姆(3)和Z = 6每配方单元28氧原子。在与晶界组合的恒定联合的基础上:Fe硫化物+ Ulvosphinel + Al-Ti-ukith Hedenbergite + Fayalite-kirschsteinite族疝,形成Tsangpoite和Matyhite,以及KuraTite(铼的Fe-类似物),可以容易地被合理化为D'Orbigny陨石形成的最后阶段的残留岩浆结晶。替代地,Tsangpoite / matyhite和配合铁硫酸盐纤维素之间的密切性关系由Fayalite + kirschsteinite ysplectite覆盖,例如与Fe硫化物中的磁铁矿+/-其他相结合的Tsangpoite成核和针状Tsangpoite的共同外向生长从Fayalite-kirschsteinite的Fealite-kirschsteinite yepercidic rim的盘状泡沫状物进入Hedenbergite,推断这些新的矿物质和晶粒边界组合可能代表由侵入偏畴和多孔橄榄石 - Plagioclase板+ Fayalite之间的反应产生的替代产品-Kirschsteinite过度生长+奥伯特+ Fe硫化物聚集体。还需要进一步的热化学和动力学证据来澄清Euhedral Tsangpoite,Matyhite和Kuratite的精确形成机制/条件,在D'Orbigny海晶的晶界。

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