Astromat

Astromaterials Data System

Data from "Origin of Iron Meteorite Groups IAB and IIICD" by Wasson et al. (1980)

Authors

John WassonJohn WillisChien WaiAlfred Kracher


Description

This dataset contains mean concentrations of Co, Ni, Cu, Ga, Ge, As, W, Ir, and Au in Groups IAB and IIICD (now Group IAB complex). Germanium was analyzed by radiochemical neutron activation analysis (RNAA) at the University of California, Los Angeles. Other elements were analyzed by instrumental neutron activation analysis (INAA) at the University of California, Los Angeles.


How To Cite

Wasson, J., Willis, J., Wai, C., Kracher, A., 2021. Data from "Origin of Iron Meteorite Groups IAB and IIICD" by Wasson et al. (1980), Version 1.0. Astromaterials Data Archive. https://doi.org/10.26022/IEDA/112040 Accessed 2026-09-29.

Download Citation from Datacite:

RISBibTex
Type

Dataset

Date Created

July 2, 2021

Size

440.32 kB

License

Download

Files

Select a file for preview.

Related Publication

Wasson, J. T., Willis, J., Wai, C. M., & Kracher, A. (1980). Origin of iron meteorite groups IAB and IIICD. Zeitschrift für Naturforschung A, 35(8), 781-795.

Funding Sources

N/A

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 RescueMeteoritesHayabusaHayabusa2Microparticle ImpactCosmic DustStardustGenesisUCLA Cosmochemistry DatabaseOSIRIS-REx
CoreTrustSeal
Certified ByCoreTrustSeal
World Data System
Regular Member ofWorld Data System
Privacy PolicyTerms of Use

© Copyright 2026 Astromaterials Data System.