Biology
Scientific paper
Dec 2011
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011agufm.p11c1604t&link_type=abstract
American Geophysical Union, Fall Meeting 2011, abstract #P11C-1604
Biology
[5112] Physical Properties Of Rocks / Microstructure, [5220] Planetary Sciences: Astrobiology / Hydrothermal Systems And Weathering On Other Planets, [6225] Planetary Sciences: Solar System Objects / Mars, [6240] Planetary Sciences: Solar System Objects / Meteorites And Tektites
Scientific paper
The nakhlite meteorites contain minerals including clays, salts and carbonates that crystallized from water within an impact-induced hydrothermal system or subsurface aquifer [1,2]. These minerals can be used to explore the longevity, scale and evolution of the aqueous system. However, such work has proven to be challenging owing to their very fine crystal size and their compositional complexity. In this study we have used a suite of techniques including CT tomography, scanning and transmission electron microscopy and Ar/Ar dating to explore the history of secondary mineralization in the nakhlites. In total there are thirteen nakhlites, however, this study has focused on Nakhla as it is the only fall. To further understand their alteration relationships we also plan to study Lafayette, MIL 003346, Yamato 000593, 000749 and NWA 5790. In contrast to previous studies that have used polished thin sections, we have examined secondary minerals exposed on freshly produced fracture surfaces from the interior of the Nakhla meteorite. This technique has revealed six textures that have not previously been described. (1) Areas of nanocrystalline/amorphous growth of sheeted silicates appearing to nucleate from underlying Cl and C rich fibrous material. (2) Underlying material which forms on the olivine grains surface with a nanoscale fibrous structure contains intergrown <5 μm sized euhedral calcium sulphate crystals. (3) The overlying sheeted silicates are also cross-cut by veins of this Cl and C enriched fibrous material. (4) A concentrically Si, Cl, Ca, Mn and Fe zoned region of alteration with a diameter of ~90 μm that has also been observed potentially sourcing enrichments from an underlying halite grain and augite and magnetite inclusions formed from symplectic exsolution in the host olivine [3]. Additionally, we have observed (5) radial growth structures emanating from halite grains and (6) etch pits in the surfaces of olivines. We will also present preliminary Ar/Ar ages for the K-bearing alteration material within the nakhlites. The textures that we have observed suggest that the sheeted silicate material formed either during fluctuations in fluid compositions or as a result of these newly discovered sites of nucleation growth from the underlying Cl and C enriched fibrous material. The presence of the fibrous material cross-cutting the silicate could indicate the following: a subsequent injection of a saline fluid, an expansion of the fibrous material rupturing the silicate, or the remobilisation of the fibrous material. The sharp contacts of the silicate with these cross cutting veins of fibrous material suggest that this material (likely brine) was exposed to only very low temperatures [4] thus not remobilising and equilibrating with the surrounding material. Some of the features that we have found would have been lost in conventional thin section manufacture and may explain why they have not been observed previously.
Lee Minchul
Lindgren Paula
Mark Darren Francis
Stuart Finlay
Tomkinson T.
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