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The H-poor nature of incompletely melted planetesimals: The view from acapulcoites and lodranites

Peterson, L, Newcombe, M, Alexander, C, , Nielsen, S(2024). The H-poor nature of incompletely melted planetesimals: The view from acapulcoites and lodranites. Geochimica et Cosmochimica Acta, 370, 1-14. https://doi.org/ https://doi.org/10.1016/j.gca.2024.02.002

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Datasets

numbertitleMethodsvariables analyzed
4Grain volatile contentsSIMSH2O, F
S2EPMA analyses and corresponding end-member mineral formulasEMP, CALCMgO, Na2O, ENSTATITE, FERROSILITE, TiO2, FeO, Cr2O3, CaO, SiO2, MnO, WOLLASTONITE, NiO, Al2O3, TOTAL, K2O, FORSTERITE, ORTHOCLASE, ANORTHITE, ALBITE
S3Grain average volatile contentsSIMSCO2, F, Cl, S, H2O
S8 Collated, corrected, and filtered SIMS H2O data for the acapulcoites and lodranites from the 01/22 and 02/22 analytical sessionsSIMSH2O

Methods

method namelaboratorymethod comment More details are available for the following variables
CALCULATEDUNKNOWNN/A
ELECTRON MICROPROBEUNIVERSITY OF MARYLANDJEOL JXA 8900R
SECONDARY ION MASS SPECTROMETRYCARNEGIE INSTITUTION WASHINGTONCameca NanoSIMS 50L. Lowest propagated uncertainty for averaged analyses due to uncertainties associated with counting statistics, SiO2 corrections, background corrections, drift corrections, and the calibration curves among averaged points

Samples

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