Beryllium‐10 and aluminum‐26 in individual cosmic spherules from Antarctica

Abstract— We present data for the cosmogenic nuclides 10 Be and 26 Al in a suite of 24 extraterrestrial spherules, collected from Antarctic moraines and deep sea sediments. All of the 10 large spherules collected in glacial till at Lewis Cliff are extraterrestrial. As in earlier work, the great majo...

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Bibliographic Details
Published in:Meteoritics
Main Authors: Nishiizumi, K., Arnold, J. R., Brownlee, D. E., Caffee, M. W., Finkel, R. C., Harvey, R. P.
Format: Article in Journal/Newspaper
Language:English
Published: Wiley 1995
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Online Access:http://dx.doi.org/10.1111/j.1945-5100.1995.tb01170.x
https://api.wiley.com/onlinelibrary/tdm/v1/articles/10.1111%2Fj.1945-5100.1995.tb01170.x
https://onlinelibrary.wiley.com/doi/pdf/10.1111/j.1945-5100.1995.tb01170.x
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Summary:Abstract— We present data for the cosmogenic nuclides 10 Be and 26 Al in a suite of 24 extraterrestrial spherules, collected from Antarctic moraines and deep sea sediments. All of the 10 large spherules collected in glacial till at Lewis Cliff are extraterrestrial. As in earlier work, the great majority of particles show prominent solar cosmic‐ray (SCR) production of 26 Al, indicating bombardment ages on the order of 10 6 years or even longer. These long ages are in direct contradiction to model ages for small particles in the inner Solar System and may require reconsideration of models of small particle lifetimes. A small fraction of the particles so far measured (6/42) possess cosmogenic radionuclide patterns consistent with predictions for meteoroid spall droplets. We believe that most of the spherules were bombarded in space primarily as bodies not much larger than their present size. The content of in situ produced 10 Be and 26 Al in quartz pebbles in the same moraine suggests that these spherules may have on average a significant terrestrial age.