NanoSIMS O isotopic analysis of a precursor silicate grains with metal core in sample OREX-800088-10
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Description
Small oliivne and other silicate and oxide phases exist within the matrix of Bennu samples. These phases are the remnants of the precursor components that formed the original Bennu parent asteroid. The oxygen isotopic composititon of these grains helps constrain the nature of what Bennu's parent formed from, and where in the protoplanetary disk this happened.
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How To Cite
Franchi, I., 2025. NanoSIMS O isotopic analysis of a precursor silicate grains with metal core in sample OREX-800088-10, Version 1.0. Astromaterials Data Archive. https://doi.org/10.60707/rs9s-7988 Accessed 2025-12-05.
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Funding Sources
This material is supported by NASA under contract NNM10AA11C issued through the New Frontiers program. Analyses were funded by STFC Grant APP72158.
