Fe isotope composition of bulk chondrules from Murchison (CM2): Constraints for parent body alteration, nebula processes and chondrule-matrix complementarity

被引:16
作者
Hezel, Dominik C. [1 ,2 ,3 ]
Wilden, Johanna S. [1 ]
Becker, Daniel [1 ]
Steinbach, Sonja [4 ]
Wombacher, Frank [1 ,3 ]
Harak, Markus [1 ]
机构
[1] Univ Cologne, Dept Geol & Mineral, Zulpicher Str 49b, D-50674 Cologne, Germany
[2] Nat Hist Museum, Dept Mineral, Cromwell Rd, London SW7 5BD, England
[3] Steinmann Inst, Meckenheimer Allee 169, D-53115 Bonn, Germany
[4] Deutsch Zentrum Luft & Raumfahrt DLR, Inst Mat Phys Weltraum, D-51147 Cologne, Germany
关键词
chondrules; matrix; Fe isotopes; tomography; chondrule formation; complementarity; STONY COSMIC SPHERULES; EARLY SOLAR NEBULA; CARBONACEOUS CHONDRITES; CV CHONDRITES; IRON; FRACTIONATION; ORIGIN; COMPONENTS; SYSTEM; METEORITES;
D O I
10.1016/j.epsl.2018.03.013
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
Chondrules are a major constituent of primitive meteorites. The formation of chondrules is one of the most elusive problems in cosmochemistry. We use Fe isotope compositions of chondrules and bulk chondrites to constrain the conditions of chondrule formation. Iron isotope compositions of bulk chondrules are so far only known from few studies on CV and some ordinary chondrites. We studied 37 chondrules from the CM chondrite Murchison. This is particularly challenging, as CM chondrites contain the smallest chondrules of all chondrite groups, except for CH chondrites. Bulk chondrules have delta Fe-56 between -0.62 and +0.24%o relative to the IRMM-014 standard. Bulk Murchison has as all chondrites a (delta Fe-56 of 0.009'00 within error. The delta Fe-56 distribution of the Murchison chondrule population is continuous and close to normal. The width of the delta Fe-56 distribution is narrower than that of the Allende chondrule population. Opaque modal abundances in Murchison chondrules is in about 67% of the chondrules close to 0 vol.%, and in 33% typically up to 6.5 vol.%. Chondrule Al/Mg and Fe/Mg ratios are sub-chondritic, while bulk Murchison has chondritic ratios. We suggest that the variable bulk chondrule Fe isotope compositions were established during evaporation and recondensation prior to accretion in the Murchison parent body. This range in isotope composition was likely reduced during aqueous alteration on the parent body. Murchison has a chondritic Fe isotope composition and a number of chondritic element ratios. Chondrules, however, have variable Fe isotope compositions and chondrules and matrix have complementary Al/Mg and Fe/Mg ratios. In combination, this supports the idea that chondrules and matrix formed from a single reservoir and were then accreted in the parent body. The formation in a single region also explains the compositional distribution of the chondrule population in Murchison. (C) 2018 Elsevier B.V. All rights reserved.
引用
收藏
页码:31 / 39
页数:9
相关论文
共 74 条
[1]   The formation conditions of chondrules and chondrites [J].
Alexander, C. M. O'D. ;
Grossman, J. N. ;
Ebel, D. S. ;
Ciesla, F. J. .
SCIENCE, 2008, 320 (5883) :1617-1619
[2]   Chemical equilibrium and kinetic constraints for chondrule and CAI formation conditions [J].
Alexander, CMO .
GEOCHIMICA ET COSMOCHIMICA ACTA, 2004, 68 (19) :3943-3969
[3]   Mass-dependent fractionation of Mg, Si, and Fe isotopes in five stony cosmic spherules [J].
Alexander, CMO ;
Taylor, S ;
Delaney, JS ;
Ma, PX ;
Herzog, GF .
GEOCHIMICA ET COSMOCHIMICA ACTA, 2002, 66 (01) :173-183
[4]   Exploration of quantitative kinetic models for the evaporation of silicate melts in vacuum and in hydrogen [J].
Alexander, CMO .
METEORITICS & PLANETARY SCIENCE, 2001, 36 (02) :255-283
[5]   Questions, questions: Can the contradictions between the petrologic, isotopic, thermodynamic, and astrophysical constraints on chondrule formation be resolved? [J].
Alexander, Conel M. O'D ;
Ebel, Denton S. .
METEORITICS & PLANETARY SCIENCE, 2012, 47 (07) :1157-1175
[6]  
ANDERS E, 1964, SPACE SCI REV, V3, P583
[7]   Geochemistry of CI chondrites: Major and trace elements, and Cu and Zn Isotopes [J].
Barrat, J. A. ;
Zanda, B. ;
Moynier, F. ;
Bollinger, C. ;
Liorzou, C. ;
Bayon, G. .
GEOCHIMICA ET COSMOCHIMICA ACTA, 2012, 83 :79-92
[8]   Formation timescales of CV chondrites from component specific Hf-W systematics [J].
Becker, Maike ;
Hezel, Dominik C. ;
Schulz, Toni ;
Elfers, Bo-Magnus ;
Muenker, Carsten .
EARTH AND PLANETARY SCIENCE LETTERS, 2015, 432 :472-482
[9]   Volatile fractionation in the early solar system and chondrule/matrix complementarity [J].
Bland, PA ;
Alard, O ;
Benedix, GK ;
Kearsley, AT ;
Menzies, ON ;
Watt, LE ;
Rogers, NW .
PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA, 2005, 102 (39) :13755-13760
[10]   Magnesium isotopic fractionation in chondrules from the Murchison and Murray CM2 carbonaceous chondrites [J].
Bouvier, Audrey ;
Wadhwa, Meenakshi ;
Simon, Steven B. ;
Grossman, Lawrence .
METEORITICS & PLANETARY SCIENCE, 2013, 48 (03) :339-353