Astromat

Astromaterials Data System

Main-group pallasites - chemical composition, relationship to IIIAB irons, and origin

Wasson, John T., Choi, Byeon-Gak(2003). Main-group pallasites - chemical composition, relationship to IIIAB irons, and origin. Geochimica et Cosmochimica Acta, 67(16), 3079-3096. https://doi.org/10.1016/S0016-7037(03)00306-5

Download Citation from Datacite:

RISBibTex

Datasets

numbertitleMethodsvariables analyzed
2Individual analyses of pallasites carried out during 1986 or more recently. Concentrations in g/g except Co and Ni (mg/g) and Sb and Re (ng/g)INAA, RNAAAu, Mo, W, Ni, Cr, Pt, As, Re, Ga, Co, Cu, Ir, Sb
1Mean concentrations of 13 elements in 33 PMG, 2 PES and 2 olivine-rich ungrouped irons (IrUn). Concentrations in g/g except Co and Ni (mg/g) and Sb and Re (ng/g)INAA, RNAAIr, Co, Cu, Pt, Sb, Au, W, Ge, Cr, Ga, As, Ni, Re
MB-CMetBase 2051 CompilationINAASb, Re, As, Pt, Ir, Cu, Co, Ge, Ni, Cr, Au, Ga

Methods

method namelaboratorymethod comment More details are available for the following variables
INSTRUMENTAL NEUTRON ACTIVATION ANALYSISUNKNOWNN/A
RADIOANALYTICAL NEUTRON ACTIVATIONUNKNOWNN/A

Samples

Back To Top
The Bubble Nebula (NGC 7635) observed by the NASA/ESA Hubble Space Telescope.
NASA Logo

Funded by NASA.
Hosted at the LDEO of Columbia University.

ArchiveStart a SubmissionSubmission GuidelinesTemplatesCuration ServicesPoliciesSearch Astromat ArchiveSearch AstroRepoArchive Overview
CollectionsLunarANGSALunar Samples Data RescueMeteoritesHayabusaMicroparticle ImpactCosmic DustStardustGenesisUCLA Cosmochemistry Database
Privacy PolicyTerms of Use

© Copyright 2025 Astromaterials Data System.