Fluid flow in chondritic parent bodies: deciphering the compositions of planetesimals |
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| Authors: | Young Ash England Rumble |
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| Institution: | Department of Earth Sciences, University of Oxford, Parks Road, Oxford, OX1 3PR, UK. Geophysical Laboratory, Carnegie Institution of Washington, 5251 Broad Branch Road NW, Washington DC, 20015, USA. |
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| Abstract: | Alteration of the Allende meteorite caused shifts in oxygen isotope ratios along a single mass fractionation line. If alteration was caused by aqueous fluid, the pattern of oxygen isotope fractionation can be explained only by flow of reactive water down a temperature gradient. Down-temperature flow of aqueous fluid within planetesimals is sufficient to explain the mineralogical and oxygen isotopic diversity among CV, CM, and CI carbonaceous chondrites and displacement of the terrestrial planets from the primordial slope 1. 00 line on the oxygen three-isotope plot. |
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