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Evolution of organic matter in Orgueil, Murchison and Renazzo during parent body aqueous alteration: In situ investigations
被引:175
作者:
Le Guillou, Corentin
[1
]
Bernard, Sylvain
[2
]
Brearley, Adrian J.
[1
]
Remusat, Laurent
[2
]
机构:
[1] Univ New Mexico, Dept Earth & Planetary Sci, Albuquerque, NM 87131 USA
[2] MNHN, CNRS, UMR 7202, Lab Mineral & Cosmochim Museum, F-75231 Paris 05, France
基金:
美国国家科学基金会;
关键词:
FINE-GRAINED RIMS;
X-RAY-ABSORPTION;
ION-BEAM FIB;
CARBONACEOUS CHONDRITE;
AMINO-ACIDS;
ISOTOPIC COMPOSITION;
SOLAR-SYSTEM;
NEXAFS SPECTROSCOPY;
INTERPLANETARY DUST;
PREBIOTIC SYNTHESIS;
D O I:
10.1016/j.gca.2013.11.020
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:
Chondrites accreted the oldest solid materials in the solar system including dust processed in the protoplanetary disk and diverse organic compounds. After accretion, asteroidal alteration may have impacted organic particles in various ways. To constrain these processes, we conducted a comprehensive study of organics disseminated within the matrices of the three carbonaceous chondrite falls, Renazzo (CR2), Murchison (CM2) and Orgueil (CI). By combining synchrotron-based STXM and TEM analyses on FIB sections of samples previously characterized by NanoSIMS, we investigated the influence of aqueous alteration on the morphology, isotopic signature, molecular structure, spatial distribution, and mineralogical environment of the organic matter within the matrices. Two different populations of materials are distinguishable: sub-micrometric individual grains, likely dominated by insoluble compounds and diffuse organic matter, finely interspersed within phyllosilicates and/or (amorphous) nanocarbonates at the nanometer scale. We suggest that this latter component, which is depleted in aromatics and enriched in carboxylic functional groups, may be dominated by soluble compounds. Organic matter in Renazzo (CR) mainly consists of chemically-homogeneous individual grains surrounded by amorphous and nanocrystalline phyllosilicates. Evidence of connectivity between organic grains and fractures indicates that redistribution has occurred: some areas containing diffuse organic matter can be observed. This diffuse organic component is more abundant in Murchison (CM) and Orgueil (CI). This is interpreted as resulting from fluid transport at the micrometer scale and encapsulation within recrystallized alteration phases. In contrast to Renazzo, organic grains in Murchison and Orgueil display strong chemical heterogeneities, likely related to chemical evolution during aqueous alteration. The observations suggest that the altering fluid was a brine with elevated concentrations of both organic and inorganic soluble components. Ultimately, when water was consumed by aqueous alteration reactions or lost from the system, soluble organic compounds accumulated in the immediate vicinity of the precipitated carbonates and phosphates. Additionally, the nanometer scale organic/phyllosilicate relationships provide a petrological environment where some of the initially accreted organic matter could have been modified through clay-mediated reactions. (C) 2013 Elsevier Ltd. All rights reserved.
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页码:368 / 392
页数:25
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