Revisiting 26Al-26Mg systematics of plagioclase in H4 chondrites

Zinner and Göpel (, ) found clear evidence for the former presence of 26Al in the H4 chondrites Ste. Marguerite and Forest Vale. They assumed that the 26Al‐26Mg systematics of these chondrites date “metamorphic cooling of the H4 parent body.” Plagioclase in these chondrites can have very high Al/Mg...

Full description

Saved in:
Bibliographic Details
Published inMeteoritics & planetary science Vol. 49; no. 6; pp. 929 - 945
Main Authors Telus, M., Huss, G. R., Nagashima, K., Ogliore, R. C.
Format Journal Article
LanguageEnglish
Published Hoboken Blackwell Publishing Ltd 01.06.2014
Wiley Subscription Services, Inc
Online AccessGet full text

Cover

Loading…
More Information
Summary:Zinner and Göpel (, ) found clear evidence for the former presence of 26Al in the H4 chondrites Ste. Marguerite and Forest Vale. They assumed that the 26Al‐26Mg systematics of these chondrites date “metamorphic cooling of the H4 parent body.” Plagioclase in these chondrites can have very high Al/Mg ratios and low Mg concentrations, making these ion probe analyses susceptible to ratio bias, which is inversely proportional to the number of counts of the denominator isotope (Ogliore et al. ). Zinner and Göpel () used the mean of the ratios to calculate the isotope ratios, which exacerbates this problem. We analyzed the Al/Mg ratios and Mg isotopic compositions of plagioclase grains in thin sections of Ste. Marguerite, Forest Vale, Beaver Creek, and Sena to evaluate the possible influence of ratio bias on the published initial 26Al/27Al ratios for these meteorites. We calculated the isotope ratios using total counts, a less biased method of calculating isotope ratios. The results from our analyses are consistent with those from Zinner and Göpel (), indicating that ratio bias does not significantly affect 26Al‐26Mg results for plagioclase in these chondrites. Ste. Marguerite has a clear isochron with an initial 26Al/27Al ratio indicating that it cooled to below 450 °C 5.2 ± 0.2 Myr after CAIs. The isochrons for Forest Vale and Beaver Creek also show clear evidence that 26Al was alive when they cooled, but the initial 26Al/27Al ratios are not well constrained. Sena does not show evidence that 26Al was alive when it cooled to below the Al‐Mg closure temperature. Given that metallographic cooling rates for Ste. Marguerite, Forest Vale, and Beaver Creek are atypical (>5000 °C/Myr at 500 °C) compared with most H4s, including Sena, which have cooling rates of 10–50 °C/Myr at 500 °C (Scott et al. ), we conclude that the Al‐Mg systematics for Ste. Marguerite, Forest Vale, and Beaver Creek are the result of impact excavation of these chondrites and cooling at the surface of the parent body, instead of undisturbed cooling at depth in the H chondrite parent body, like many have assumed.
Bibliography:ArticleID:MAPS12304
istex:25A7E0E534418918708BF856452A86907312E351
ark:/67375/WNG-8FNQVN0Q-Q
Table S1: Composition (in wt.%) of anorthite, oligoclase, olivine, pyroxene, and chromite grains from Ste. Marguerite. Table S2: Composition (in wt.%) of anorthite, oligoclase, olivine, pyroxene, and chromite grains from Forest Vale. Table S3: Composition (in wt.%) of oligoclase, olivine, pyroxene, and chromite grains from Beaver Creek. Table S4: Composition (in wt.%) of oligoclase, olivine, pyroxene, and chromite grains from Sena.
NASA NESSF - No. NNX11AN62H; No. NNX11AG78G
ISSN:1086-9379
1945-5100
DOI:10.1111/maps.12304