Elemental abundance anomalies in the late Cenomanian extinction interval - A search for the source(s)

Details Elemental abundance anomalies in the late Cenomanian extinction interval - A search for the source(s) Elemental abundance anomalies in the late Cenomanian extinction interval - A search for the source(s)

May 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993e%26psl.117..189o&link_type=abstract

Earth and Planetary Science Letters (ISSN 0012-821X), vol. 117, no. 1-2, p. 189-204.

Computer Science

16

Abundance, Chemical Elements, Cretaceous Period, Trace Elements, Neutron Activation Analysis, Planetary Composition, Sea Level, Structural Basins

Scientific paper

Measurements of elemental abundances by neutron activation methods across the Cenomanian-Turonian extinction interval in samples collected from 16 sites in the Western Interior Basin of North America from 12 widely separated locations around the globe, including six ODP/DSDP sites, are reported. In most Western Interior Basin sites, in Colombia, and in Western Europe, two closely spaced elemental abundance peaks occur in the upper Cenomanian (about 92 m.y.), spanning the ammonite zones of Sciponoceras gracile through Neocardioceras juddii. Elements with anomalously high concentrations include Sc, Ti, V, Cr, Mn, Co, Ni, Ir, Pt, and Au. The lower peak coincides with the disappearance (extinction) of the foraminifer Rotalipora cushmani. In North American sections R. greenhornensis also disappears at or just below this horizon, but in Europe it disappears considerably earlier than R. cushmani. Although the weak geochemical signal from comet impact(s) could be masked by the strong terrestrial-like overprint, these anomalies more likely resulted in the large late Cenomanian through early Turonian eustatic rise and deep-water opening of the South Atlantic.

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