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Noble Metal Enrichments in Cosmic Spherules

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Origin and Evolution of Interplanetary Dust

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 173))

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Abstract

In this work, studies on relationships of chemical compositions between fusion crust and nucleus in iron spherules are reported. More than 10% of the iron spherules which were picked out from deep sea sediment, have cores and crusts. We were able to divide three of them into cores and crusts. Each cores and crusts were analyzed individually by INAA. The core mainly consists of iron and nickel. Other trace elements, especially noble metal Au and Ir were concentrated in the core. The mechanism of core formation in the iron spherules shows us the origin of them.

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References

  • Brownlee D.E., Bates B.A. and Wheelock M.M., (1984) ‘Extraterrestrial platinum group nuggets in deep-sea sediments’, Nature, 309, 693–695

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  • Yamakoshi K. (1984) ‘Chemical compositions of magnetic spherules from deep-sea sediments determined by instrumental neutron activation analysis’, Geochemical J.. 18. 147–152

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© 1991 Springer Science+Business Media Dordrecht

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Nogami, K., Misawa, K., Omori, R., Jianguo, M., Yamakoshi, K. (1991). Noble Metal Enrichments in Cosmic Spherules. In: Levasseur-Regourd, A.C., Hasegawa, H. (eds) Origin and Evolution of Interplanetary Dust. Astrophysics and Space Science Library, vol 173. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-3640-2_22

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  • DOI: https://doi.org/10.1007/978-94-011-3640-2_22

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-5616-8

  • Online ISBN: 978-94-011-3640-2

  • eBook Packages: Springer Book Archive

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