Beryllium-10 and Aluminum-26 in Individual Cosmic Spherules from Antarctica

K. Nishiizumi, J. Arnold, D. Brownlee, M. Caffee, R. Finkel, R. Harvey
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引用次数: 23

Abstract

— We present data for the cosmogenic nuclides 10Be and 26Al 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 26Al, indicating bombardment ages on the order of 106 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 10Be and 26Al in quartz pebbles in the same moraine suggests that these spherules may have on average a significant terrestrial age.
来自南极洲的单个宇宙球体中的铍-10和铝-26
-我们提供了从南极冰碛和深海沉积物中收集的一套24个地外球体中的宇宙成因核素10Be和26Al的数据。在刘易斯悬崖冰川上收集到的10个大球体都是外星生物。在早期的研究中,绝大多数粒子显示出明显的太阳宇宙射线(SCR)产生的26Al,表明轰击年龄在106年甚至更长。这些很长的年龄与太阳系内部小粒子的年龄模型直接矛盾,可能需要重新考虑小粒子寿命模型。迄今为止测量到的一小部分粒子(6/42)具有与流星体碎片液滴预测一致的宇宙成因放射性核素模式。我们相信,大多数小球体在太空中受到撞击时,最初还是比它们现在的大小大不了多少的物体。同一冰碛石英石中原位产生的10Be和26Al含量表明,这些球粒可能具有明显的地球平均年龄。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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