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O18/O16 and C13/C12 Ratios of Fossils from the Hot-Brine Deep Area of the Central Red Sea

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Hot Brines and Recent Heavy Metal Deposits in the Red Sea

Abstract

Carbon and oxygen isotope ratios of foraminifera and pteropod shells show considerable fluctuations with depth in all cores investigated. Distinct changes in the isotope ratios at certain depths can be correlated among cores. Foraminifera tests deposited in the Discovery and Atlantis II Deeps during the last 10,000 years show evidence of a beginning isotopic re-equilibration with the hot brine. Older deposits show no such effect, suggesting a maximum age of the brine of about 10,000 years. The isotopic data strongly suggest the repeated occurrence of periods of evaporation in the Red Sea during the last 80,000 to 100,000 years. It seems likely that these periods coincided with those of lowered sea level which severely restricted the exchange of water between the Red Sea and the Indian Ocean. Alternatively the reduced exchange could have been caused by tectonic activity near the Strait of Bab el Mandeb.

Woods Hole Oceanographic Institution Contribution No. 2195.

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Deuser, W.G., Degens, E.T. (1969). O18/O16 and C13/C12 Ratios of Fossils from the Hot-Brine Deep Area of the Central Red Sea. In: Degens, E.T., Ross, D.A. (eds) Hot Brines and Recent Heavy Metal Deposits in the Red Sea. Springer, Berlin, Heidelberg. https://doi.org/10.1007/978-3-662-28603-6_34

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  • DOI: https://doi.org/10.1007/978-3-662-28603-6_34

  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-662-27120-9

  • Online ISBN: 978-3-662-28603-6

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