The mineralogy and alteration history of the Yamato-type (CY) carbonaceous chondrites

被引:19
作者
Suttle, M. D. [1 ,2 ]
King, A. J. [2 ]
Harrison, C. S. [2 ]
Chan, Q. H. S. [1 ,3 ]
Greshake, A. [4 ]
Bartoschewitz, R. [5 ]
Tomkins, A. G. [6 ]
Salge, T. [7 ]
Schofield, P. F. [2 ]
Russell, S. S. [2 ]
机构
[1] Open Univ, Sch Phys Sci, Walton Hall, Milton Keynes MK7 6AA, England
[2] Nat Hist Museum, Planetary Mat Grp, Cromwell Rd, London SW7 5BD, England
[3] Royal Holloway Univ London, Dept Earth Sci, Egham TW20 0EX, Surrey, England
[4] Leibniz Inst Evolut & Biodiversitatsforsch, Museum Naturkunde, Invalidenstr 43, D-10115 Berlin, Germany
[5] Bartoschewitz Meteorite Lab, Weiland 37, D-38518 Gifhorn, Germany
[6] Sch Earth Atmosphere & Environm, Melbourne, Vic, Australia
[7] Nat Hist Museum, Imaging & Anal Ctr, Cromwell Rd, London SW7 5BD, England
关键词
Carbonaceous chondrites; C-type asteroids; CY chondrites; Aqueous alteration; Thermal metamorphism; INSOLUBLE ORGANIC-MATTER; TAGISH LAKE METEORITE; AQUEOUS ALTERATION; OXYGEN-ISOTOPE; PARENT BODY; RAMAN-SPECTROSCOPY; CM CHONDRITES; AMORPHOUS SILICATES; INTERPLANETARY DUST; MODAL MINERALOGY;
D O I
10.1016/j.gca.2023.09.024
中图分类号
P3 [地球物理学]; P59 [地球化学];
学科分类号
0708 ; 070902 ;
摘要
The CY chondrites are a group of thermally metamorphosed carbonaceous chondrites. Although they share similarities with the CM and CI chondrites, their primary properties argue for a distinct classification. Previous studies have highlighted their isotopically heavy bulk compositions (delta O-17 = 10 parts per thousand, delta O-18 = 21 parts per thousand, Delta O-17 = 0 parts per thousand) and exceptionally high sulphide abundances (10-30 vol%). In this work we explore their petrography and alteration history. The CYs accreted low abundances of chondrules (15-20 area%) with average apparent diameters slightly larger (similar to 320-340 mu m) than the CM chondrites. In contrast to the CMs, the CYs record an early episode of brecciation prior to the main window of aqueous alteration. Subsequent fluid activity produced a range of alteration extents with both CY2 and CY1 chondrites documented. Phyllosilicate minerals in the CYs were a mix of serpentine and saponite (including occurrences of Na-saponite) with minor quantities of chlorite (within chondrules). An initial generation of Fe-sulphides formed by sulfidation of metal, and by precipitation from S-rich fluids. Three generations of carbonates are recognized, an early generation that infilled voids left by brecciation and co-precipitated with sulphide, a later generation that co-precipitated with magnetite and a final Fe-Mg-bearing generation which formed large (>100 mu m) clasts. Only the first-generation carbonates are found in the CY2s, while the CY1s preserve all three generations. Phosphates occur as Ca-apatite or rarely as Mg-bearing apatite and have hydroxylapatite compositions, indicating low halogen activities in the alteration fluids. Refractory oxides (ilmenite and Cr-spinel) occur as precipitates adhering to the margins of phyllosilicates. They formed late in the alteration sequence and attest to oxidizing conditions. During the late-stages of aqueous alteration Fe-sulphides were replaced by magnetite. Thermal metamorphism (Stage II-IV: similar to 300-750 degrees C) overprinted aqueous alteration leading to dehydration and recrystallization of the phyllosilicate matrix and the decomposition of some carbonate phases. Most Fe-sulphide grains survived heating without decomposition as initial partial decomposition from pyrrhotite to troilite under closed system conditions led to elevated S-2 gas and resulted in a stabilizing effect. Retrograde reactions between trapped S-2 gas and metal/magnetite formed a final generation of Fe-sulphides. The survival of Fe-sulphides and their stochiometric troilite compositions are evidence for near-closed system heating. Analysis of organic matter by Raman spectroscopy supports an interpretation of short-duration heating (on the scale of minutes to days), at peak temperatures between 750 and 900 degrees C. Thus, an impact event was the most likely cause of metamorphic heating.
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页码:245 / 264
页数:20
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