Origin of fabrics and olivine chemical variations preserved in brachinite and brachinite‐like achondrite meteorites
Gruber, Benjamin H., Nicklas, Robert W., Day, James M. D., , Bernard, Rachel E.(2024). Origin of fabrics and olivine chemical variations preserved in brachinite and brachinite‐like achondrite meteorites. Meteoritics & Planetary Science, Online Version of Record. https://doi.org/10.1111/maps.14179
Datasets
| number | title | Methods | variables analyzed | ||
|---|---|---|---|---|---|
| S1 | Major element abundances in mineral phases determined by EPMA (wt%) | EMP | TOTAL, Co, Fe, S, Ni, FeO, CaO, MgO, MnO, SiO2, Cr2O3, TiO2, NiO, Na2O, Al2O3, K2O, Zn, Cu, CoO | ||
| S2 | Major and trace element abundances in mineral phases determined by LAICPMS | LA-ICPMS | V, Fe, Na, Y, Mg, Sc, Co, Ca, Al, Ti, Ni, Zr, Ga | ||
Methods
| method name | laboratory | method comment | More details are available for the following variables | |
|---|---|---|---|---|
| ELECTRON MICROPROBE | UNIVERSITY OF NEVADA LAS VEGAS | JEOL JXA-8900, 15kV, 20nA, 2 micrometer spot size | ||
| LASER ABLATION INDUCTIVELY COUPLED PLASMA MASS SPECTROMETRY | SCRIPPS INSTITUTION OF OCEANOGRAPHY | New Wave UP213 (213 nm) laser ablation system coupled to a Thermo Scientific iCAPq Qc |
