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Published August 1995 | public
Journal Article

Fractionation of ruthenium from iridium at the Cretaceous-Tertiary boundary

Abstract

New data on Ru/Ir abundance ratios are presented for nonmarine (Hell Creek, Montana; Frenchman River, Saskatchewan) and marine Cretaceous-Tertiary boundary sites (Brazos River, Texas; Beloc, Haiti; DSDP 577 and DSDP 596). The Ru/Ir ratio varies from 0.5 to 1 within 4000 km of Chicxulub and increases to 2–3 at paleodistances (65 Ma) of up to 12,000 km from the impact site. For CI chondrites, Ru/Ir= 1.5. A ballistic model of ejecta cloud cooling and expansion, which employs the available vapor-pressure versus temperature data for Ru and Ir, predicts qualitatively similar global variation in the Ru/Ir ratio but by only a factor of 1.5. We infer that several other factors, such as remobilization of PGE during diagenesis, preferential oxidation of Ru, condensation kinetics and atmospheric chemical and circulation processes, may account for the observed larger Ru/Ir variation.

Additional Information

© 1995 Elsevier Science B.V. Received 10 November 1994; accepted 12 June 1995. We are grateful to A. Hildebrand, D. Beeson and J. Lerbekmo for providing samples. We thank the ODP for supplying samples of DSDP cores 596 and 597. We thank reviewers C. Koeberl, F. Asaro and G. Ravizza, who made numerous suggestions which we believe improved this paper. Discussions with L. Watson, M. Hirschmann, W. W. Anderson and B. McInnes also improved the paper. This research was supported in Canada by NSERC and in the USA by NASA. We are grateful for paleoreconstruction provided by the Plates Project, Institute for Geophysics, The University of Texas, Austin. This is contribution 5446 of the Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, California. [MK]

Additional details

Created:
August 20, 2023
Modified:
October 18, 2023