Astromat

Astromaterials Data System

40Ar-39Ar ages of H-chondrite impact melt breccias

Swindle, Timothy D., Isachsen, Clark E., Weirich, John R., Kring, David A.(2009). 40Ar-39Ar ages of H-chondrite impact melt breccias. Meteoritics & Planetary Science, 44(5). https://doi.org/10.1111/j.1945-5100.2009.tb00766.x

Download Citation from Datacite:

RISBibTex

Datasets

numbertitleMethodsvariables analyzed
1Estimated ages of events recorded by H chondrites from this studyAR_ARAGE
2Ages of heavily-shocked or shock-melted H chondritesAR_ARAGE

Methods

method namelaboratorymethod comment More details are available for the following variables
AR40_AR39 AGE DETERMINATIONUNIVERSITY OF ARIZONAAll irradiations were at the University of Michigan Ford Reactor. J factors were (7.61 ± 0.06) × 10−2 for Ourique, (1.968 ± 0.024) × 10−2 for Gao-Guenie, NWA 2058, and LAP 02240, and (2.144 ± 0.004) × 10−3 for the other LaPaz meteorites. In all irradiation packages, samples of MMhb-1 hornblende were included as the primary irradiation monitor, while samples of CaF2 and K2SO4 were included to monitor interfering reactions producing various Ar isotopes from Ca and K, respectively

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 RescueMeteoritesHayabusaHayabusa2Microparticle ImpactCosmic DustStardustGenesisUCLA Cosmochemistry DatabaseOSIRIS-REx
Privacy PolicyTerms of Use

© Copyright 2025 Astromaterials Data System.