New age for ferromanganese crust 109D-C and implications for isotopic records of lead, neodymium, hafnium, and thallium in the Pliocene Indian Ocean

New age for ferromanganese crust 109D-C and implications for isotopic records of lead, neodymium, hafnium, and thallium in the Pliocene Indian Ocean

This study presents a high‐resolution record of osmium and thallium isotopes in a ferro‐manganese (Fe‐Mn) crust from the Indian Ocean, Antipode 109D‐C. These results, when combined with additional new Os isotope data from ODP Hole 756B in the southeast Indian Ocean, define a new best estimate for th...

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Bibliographic Details
Published in:Paleoceanography Vol. 26; no. 2; pp. np - n/a
Main Authors: Nielsen, Sune G., Gannoun, Abdelmouhcine, Marnham, Charles, Burton, Kevin W., Halliday, Alex N., Hein, James R.
Format: Journal Article
Language:English
Published: Washington Blackwell Publishing Ltd 01-06-2011
American Geophysical Union
Subjects:
Age
Deep water
Earth Sciences
Environmental Sciences
ferromanganese crust
Geochemistry
Global Changes
Hafnium
Isotopes
Manganese
Marine
Neodymium
Ocean basins
Ocean bottom
Ocean circulation
Oceanic crust
Oceans
Osmium
osmium isotopes
Pliocene
Sciences of the Universe
Thallium
thallium isotopes
Water circulation
ISW, Indian Ocean
I, Pacific
AN, North Atlantic, North Atlantic Deep Water
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Summary:This study presents a high‐resolution record of osmium and thallium isotopes in a ferro‐manganese (Fe‐Mn) crust from the Indian Ocean, Antipode 109D‐C. These results, when combined with additional new Os isotope data from ODP Hole 756B in the southeast Indian Ocean, define a new best estimate for the age at the base of this crust of ∼6.5 Ma, which is significantly different from a previous estimate of ∼15 Ma based on Co‐flux modeling. The Tl isotope record obtained for the Indian Ocean resembles that for the Pacific Ocean with a small but well‐defined increase occurring over the last ∼5 Myr. This contrasts with two records from the Atlantic Ocean which do not have resolvable variations. Ocean basin–scale Tl isotope variation may be inconsistent with the inferred modern marine residence time for Tl of ∼20 kyr but could be explained by an increase in ocean crust production rates in the Pacific and Indian oceans since ∼10 Ma. The improved age model for 109D‐C reveals that the Hf isotope composition of Indian Ocean bottom waters has remained homogenous over the last ∼6 Myr. Thus, this isotope system does not bear any evidence that the influence of North Atlantic Deep Water in the formation of Indian Ocean bottom waters has changed during that time. However, because of the lack of knowledge about Hf isotopes as a tracer of ocean circulation, we cannot conclude that export of NADW decreased over the last 6 Myr. Key Points Redefine the age of Fe‐Mn crust 109D‐C from Indian Ocean Thallium isotopes in Indian and Pacific identical over last 5 Myr Radiogenic isotopes in 109D‐C cannot be used to infer influence of NADW
Bibliography:ark:/67375/WNG-797206MW-P
ArticleID:2010PA002003
Tab-delimited Table 1.Tab-delimited Table 2.
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ObjectType-Article-1
SourceType-Scholarly Journals-1
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content type line 23
ISSN:0883-8305
2572-4517
1944-9186
2572-4525
DOI:10.1029/2010PA002003