Abstract
THE recent detection of aluminium-26 in marine sediments by Amin, Kharkar and Lal1 has posed a question about the origin of this nuclide. Lal and Venkatavaradan2 pointed out that the amount of aluminium-26 in sediments is an order of magnitude higher than expected, as a result of its production by cosmic ray interactions in the terrestrial environment. Thus they concluded that the large amount of aluminium-26 can only be explained by postulating an influx with extraterrestrial cosmic dust which has been exposed to a significant flux of energetic particles capable of producing nuclear interactions.
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References
Amin, B. S., Kharkar, D. P., and Lal, D., Deep-Sea Res., 13, 805 (1966).
Lal, D., and Venkatavaradan, V. S., Science, 151, 1381 (1966).
Yiou, F., Baril, M., Dufaure de Citres, J., Fontes, P., Gradsztajn, E., and Bernas, R., Phys. Rev. (in the press).
Lal, D., and Peters, B., in Handbuch der Physik, 46/2 (Springer, Berlin, 1967).
Honda, M., and Lal, D., Nucl. Phys., 51, 363 (1964).
Reeves, H., J. Physiq. (suppl.), colloque No. 1, Cl, 28 (1966).
Nilsson, C., Science, 153, 1242 (1966).
Goldberg, E. D., and Koide, M., Geochim. Cosmochim. Acta, 26, 417 (1962).
Teh-Lung Ku, thesis, Columbia Univ. (1966).
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YOKOYAMA, Y. Terrestrial Origin of Aluminium-26 and Oceanic Sedimentation Rate. Nature 216, 569–571 (1967). https://doi.org/10.1038/216569a0
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DOI: https://doi.org/10.1038/216569a0
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