Isotopic fractionation of iron, potassium, and oxygen in stony cosmic spherules: Implications for heating histories and sources

被引:63
作者
Taylor, S
Alexander, CMO
Delaney, J
Ma, P
Herzog, GF
Engrand, C
机构
[1] CRREL, Hanover, NH 03755 USA
[2] Dept Terr Magnetism, Washington, DC 20001 USA
[3] Rutgers State Univ, Dept Geol Sci, Piscataway, NJ 08854 USA
[4] Rutgers State Univ, Dept Chem & Biol Chem, Piscataway, NJ 08854 USA
[5] CSNSM, F-91405 Orsay, France
基金
美国国家科学基金会; 美国国家航空航天局;
关键词
D O I
10.1016/j.gca.2004.11.027
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
Atmospheric heating alters the compositions and textures of micrometeorites. To understand the changes and to test a proposed relationship between a micrometeorite's petrographic texture and its degree of heating, we made elemental and multiple isotope analyses of stony cosmic spherules (sCS) collected from the South Pole Water well. Specifically, we analyzed the elemental compositions of 94 sCS and the isotopic ratios of Fe, K and O, on 43, 12 and 8 of these sCS, respectively. Our results show that sCS classified as strongly heated generally have lower concentrations of volatile and moderately volatile elements. Of the 43 spherules analyzed for Fe isotopes, only 5 have delta(57)Fe >5 parts per thousand. In contrast, enrichment of K-41 is pervasive (delta(41)K > 0 in all 12 spherules analyzed) and large (up to 183 parts per thousand). The determination of K isotope abundances in sCS may therefore be useful in deciphering thermal histories. Three of the eight sCS analyzed for O isotopes are mass fractionated with delta(18)O > 30 parts per thousand. We attribute two of these three delta(18)O enrichments to evaporative losses of oxygen in the atmosphere and the third to the presence in the parent material of an exotic phase, perhaps a sulfate or a carbonate. The K isotope and O isotope data are broadly consistent with the proposed textural classification. Because most spherules were not heated enough to fractionate Al, Mg, or Si, we compared the measured Mg/Al and Si/Al ratios directly to those of conventional meteorites and their matrices. similar to 30% of the sCS have compositions outside the range defined by the bulk and the matrix compositions of known meteorite groups but consistent with those of pyroxene- and olivine-rich materials and may be samples of chondrules. The other 70% have Mg/Al and Si/Al ratios similar to those of Cl, CM, CO, and CV chondrites. Natural variability of the Mg/Al and Si/Al ratios precludes the assignment of an individual sCS to a particular class of C-chondrite. Copyright (c) 2005 Elsevier Ltd.
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收藏
页码:2647 / 2662
页数:16
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