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Evolution Of Water Reservoirs In The Early Solar System Through Their Oxygen Isotopic Composition

Baker, Lee (2001). Evolution Of Water Reservoirs In The Early Solar System Through Their Oxygen Isotopic Composition. PhD thesis The Open University.

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A new technique has been developed to enable analyses of δ170 and δ180 from small water samples extracted from meteorites. Isotopic measurements are made using a continuous-flow, isotope ratio mass spectrometer (Delta C, Finnigan Mat) utilising a helium carrier gas. Oxygen is extracted from water using the powdered, solid fluorinating agent CoF3, and is purified using a GC column (PLOT, 5Å). Reproducibility of the method, determined using solid standards and reference waters is ±.30%c for δ18O and +0.14%c for ΔI7O (1σ in each case). The technique has been applied to three suites of meteorites: Carbonaceous chondrites (CI and CM), SNC meteorites (four meteorites) and a selection of Antarctic samples, three eucrites and one ordinary chondrite. Results were used to constrain models of the origin of Solar System water and its subsequent interaction on the meteorite parent bodies. Results from carbonaceous chondrites suggest that water accreting to bodies in the early Solar System was enriched in both 17O and 18O and had a Δ170 of at least +2%c The isotopic composition of water evolved during hydrothermal alteration on parent bodies toward lower Δ17O values, more similar to that of the host rocks. The complex release profile indicate that these meteorites experienced several periods of hydrothermal activity. SNC sample results have suggested the presence of two isotopically distinct reservoirs, the silicate crust and the hydrosphere each possessing distinct Δ170 values. A third component with a large 17O excess (+4%) was detected in ALH84001. The magnitude of this anomaly indicates an origin due to heterogeneous accretion or late stage veneer and cannot be produced by hydrodynamic escape. Results from the eucrites and ordinary chondrite also suggested isotopically distinct parent body silicate and hydrous reservoirs and may also be consistent with widespread late input of isotopically distinct water in the Solar System.

Item Type: Thesis (PhD)
Copyright Holders: 2001 The Author
Keywords: meteorites; dissolved oxygen; oxygen isotopes; solar system
Academic Unit/School: Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Item ID: 19051
Depositing User: Ann McAloon
Date Deposited: 30 Nov 2009 12:27
Last Modified: 02 May 2018 13:06
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