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Oxygen isotope systematics of chondrules in the Allende CV3 chondrite: High precision ion microprobe studies
被引:103
|作者:
Rudraswami, N. G.
[1
]
Ushikubo, T.
[1
]
Nakashima, D.
[1
]
Kita, N. T.
[1
]
机构:
[1] Univ Wisconsin, Dept Geosci, WiscSIMS, Madison, WI 53706 USA
基金:
美国国家科学基金会;
关键词:
MAGNESIAN CHONDRULES;
RELICT OLIVINE;
SOLAR NEBULA;
ORIGIN;
RESERVOIRS;
DURATION;
SPINEL;
AL-26;
FRACTIONATION;
HETEROGENEITY;
D O I:
10.1016/j.gca.2011.09.035
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 oxygen three-isotope systematics of 36 chondrules from the Allende CV3 chondrite are reported using high precision secondary ion mass spectrometer (CAMECA IMS-1280). Twenty-six chondrules have shown internally homogenous Delta O-17 values among olivine, pyroxene, and spinel within a single chondrule. The average Delta O-17 values of 19 FeO-poor chondrules (13 porphyritic chondrules, 2 barred olivine chondrules, and 4 chondrule fragments) show a peak at -5.3 +/- 0.6 parts per thousand (2SD). Another 5 porphyritic chondrules including both FeO-poor and FeO-rich ones show average Delta O-17 values between -3 parts per thousand and -2 parts per thousand, and 2 other FeO-poor barred olivine chondrules show average Delta O-17 values of -3.6 parts per thousand and 0 parts per thousand. These results are similar to those for Acfer 094 chondrules, showing bimodal Delta O-17 values at -5 parts per thousand and -2 parts per thousand. Nine porphyritic chondrules contain olivine grains with heterogeneous Delta O-17 values as low as -18 parts per thousand, indicating that they are relict olivine grains and some of them were derived from precursors related to refractory inclusions. However, most relict olivine grains show oxygen isotope ratios that overlap with those in homogeneous chondrules. The Delta O-17 values of four barred olivine chondrules range from -5 parts per thousand to 0 parts per thousand, indicating that not all BO chondrules plot near the terrestrial fractionation line as suggested by previous bulk chondrule analyses. Based on these data, we suggest the presence of multiple oxygen isotope reservoirs in local dust-rich protoplanetary disk, from which the CV3 parent asteroid formed. A compilation of 225 olivine and low-Ca pyroxene isotopic data from 36 chondrules analyzed in the present study lie between carbonaceous chondrite anhydrous mineral (CCAM) and Young and Russell lines. These data define a correlation line of delta O-17 = (0.982 +/- 0.019) x delta O-18 - (2.91 +/- 0.10), which is similar to those defined by chondrules in CV3 chondrites and Acfer 094 in previous studies. Plagioclase analyses in two chondrules plot slightly below the CCAM line with Delta O-17 values of -2.6 parts per thousand, which might be the result of oxygen isotope exchange between chondrule mesostasis and aqueous fluid in the CV parent body. (C) 2011 Elsevier Ltd. All rights reserved.
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页码:7596 / 7611
页数:16
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