Grossmanite, CaTi3+AlSiO6, a new pyroxene from the Allende meteorite
نویسندگان
چکیده
Grossmanite, Ca(Ti,Mg,Ti)AlSiO6 with an end-member formula CaTiAlSiO6, is a new member of the Ca clinopyroxene group, where the trivalent cations are dominant in the M1 site with Ti3+ being the dominant trivalent cation. It occurs as micrometer-sized crystals along with spinel and perovskite in a melilite host in Ca-,Al-rich refractory inclusions from the Allende meteorite. The mean chemical composition determined by electron microprobe analysis of the type material is (wt%) SiO2 27.99, Al2O3 24.71, CaO 24.58, Ti2O3 10.91, TiO2 6.68, MgO 4.45, Sc2O3 0.43, V2O3 0.19, ZrO2 0.13, FeO 0.08, Cr2O3 0.03, sum 100.20. Its empirical formula calculated on the basis of 6 O atoms is Ca1.00[(Ti 0.35 Al0.18Sc0.01V 0.01)Σ0.55Mg0.25Ti 0.19]Σ1.00(Si1.07Al0.93)Σ2.00O6. Grossmanite is monoclinic, C2/c; a = 9.80 Å, b = 8.85 Å, c = 5.36 Å, β = 105.62°, V = 447.70 Å3, and Z = 4. Its electron back-scatter diffraction pattern is an excellent match to that of Ti3+-rich pyroxene with the C2/c structure. The five strongest calculated X-ray powder diffraction lines are [d spacing in Å, (I), hkl] 2.996 (100) (221), 2.964 (31) (310), 2.581 (42) (002), 2.600 (28) (131), 2.535 (47) (221). The name is for Lawrence Grossman, a cosmochemist at the University of Chicago.
منابع مشابه
BURNETTITE, CaVAlSiO6, AND PAQUEITE, Ca3TiSi2(Al2Ti)O14, TWO NEW MINERALS FROM ALLENDE: CLUES TO THE EVOLUTION OF A V-RICH Ca-Al-RICH INCLUSION
Introduction: During a nanomineralogy investigation of the Allende CV3 meteorite, we discovered two new minerals, burnettite (IMA 2013054; CaVAlSiO6) and paqueite (IMA 2013-053; Ca3TiSi2(Al2Ti)O14), in a V-rich, fluffy Type A Ca-Alrich inclusion (CAI) A-WP1 (0.6 × 1 mm in size) in USNM 7617, which was previously studied by Paque and coworkers [1-3]. Electron probe microanalysis (EPMA), scanning...
متن کاملDiscovery of natural MgSiO3 tetragonal garnet in a shocked chondritic meteorite
MgSiO3 tetragonal garnet, which is the last of the missing phases of experimentally predicted high-pressure polymorphs of pyroxene, has been discovered in a shocked meteorite. The garnet is formed from low-Ca pyroxene in the host rock through a solid-state transformation at 17 to 20 GPa and 1900° to 2000°C. On the basis of the degree of cation ordering in its crystal structure, which can be ded...
متن کاملThe Lodran meteorite and its relationship to the ureilites
Lodran is a unique meteorite consisting of roughly equal amounts of metal, olivine, and pyroxene with minor amounts of sulphide, chromite, phosphide, chrome-diopside, and a new phase with a composition close to (K,Na)A1SisO12. Zahringer reported planetary-type rare gases in both the metal and silicates, suggesting a primitive nature. The pyroxene composition is Fs13.s with little variation. Oli...
متن کاملIron Isotope Composition of Allende and Chainpur Chondrules: Effects of Equilibration and Thermal History
Introduction: We have studied the petrography and Fe-isotope composition of seven chondrules, four from the Allende (CV3) carbonaceous chondrite and three from the Chainpur (LL3.4) ordinary chondrite. Three textural-chemical chondrule types are represented within this sample set: (1) BO, (2) RP and (3) PO/POP. These textural differences allow us to exa mine the Fe-isotope composition in materia...
متن کامل4.4 Ga Alteration of Chondrules in Allende (cv3) Parent Body: Evidence from the Rb-sr System
Introduction: It has been revealed that both of the thermal and aqueous alteration had occurred in the CV parent body [1, 2, 3]. To give a constraint to the alteration processes, the Allende meteorite can be a best example, because the following results indicate that the Allende is the strongest altered meteorite among the CV chondrites, those are: (a) homogeneity of the olivine in matrix of th...
متن کامل