THE NEODYMIUM ISOTOPIC COMPOSITION OF MANGANESE NODULES FROM THE SOUTHERN AND INDIAN OCEANS, THE GLOBAL OCEANIC NEODYMIUM BUDGET, AND THEIRBEARING ON DEEP-OCEAN CIRCULATION

Citation
F. Albarede et al., THE NEODYMIUM ISOTOPIC COMPOSITION OF MANGANESE NODULES FROM THE SOUTHERN AND INDIAN OCEANS, THE GLOBAL OCEANIC NEODYMIUM BUDGET, AND THEIRBEARING ON DEEP-OCEAN CIRCULATION, Geochimica et cosmochimica acta, 61(6), 1997, pp. 1277-1291
Citations number
73
Categorie Soggetti
Geochemitry & Geophysics
ISSN journal
00167037
Volume
61
Issue
6
Year of publication
1997
Pages
1277 - 1291
Database
ISI
SICI code
0016-7037(1997)61:6<1277:TNICOM>2.0.ZU;2-8
Abstract
Manganese nodules from the Indian and Southern oceans have been analyz ed for their Nd isotope composition. The nodules of hydrogenous origin with >100 ppm Nd have epsilon(Nd) values in the range -11 to -6.5. Th e data show that the Nd isotope ratios form two geographical isotopic domains. The samples with the least radiogenic Nd (lower epsilon(Nd) v alues) are found around the southern tip of Africa where the influence of the North-Atlantic Deep Water (NADW) dominates. From the Macquarie Ridge south of Australia to the Drake Passage at South America, the A ntarctic Circumpolar Current (ACC) seems to be isotopically well mixed with more radiogenic epsilon(Nd) values in the range -6.5 to -8. Thes e values extend across the Drake Passage and the Argentine Basin, alth ough diagenetic nodules with <100 ppm in this region show a further in crease of the epsilon(Nd) values to -4 to -6. The Indian Ocean data ea st of the Madagascar Ridge display a rather small variation with epsil on(Nd) values similar to the same sector of the ACC (-6.2 to -8.0) and confirm that Nd from deep Circum-Antarctic waters dominate the Indian Ocean. Despite the small variation, slightly higher Nd isotope ratios in the eastern relative to the western Indian Ocean indicate a compon ent of Nd from deep Pacific waters flowing into the Indian Ocean. The isotopic composition of Nd in Mn nodules is usually similar to that of their ambient seawater, and the global patterns mimic the broad featu res of present-day deep ocean circulation. Because the Mn nodules as s ampled reflect the average Nd in the deep water masses over periods of 10(5)-10(6) years, the consistency with present-day seawater indicate s that the present-day patterns of deep ocean circulation predominated throughout the Pleistocene. An exception is in the Drake Passage and Argentine Basin, where more nodules are more radiogenic than the ambie nt seawater and reflect either a weakening of NADW during glacial stag es or, alternatively, a local source which is clearly present in diage netic Mn nodules from this region. The global Nd budget in the Souther n Ocean is consistent with models of geostrophic transport: Nd in the ACC can be accounted for by a mixture of unradiogenic Nd from Atlantic and radiogenic Nd from Pacific sources. The radiogenic component rele ased by volcanogenic particles in the nepheloid layer, erupted from of the peri-Pacific rim volcanoes, exerts a major influence on Pacific s eawater. The residence time of Nd in the ACC is estimated to be 70 yea rs. Mixing therefore requires more than one revolution around Antarcti ca. Copyright (C) 1997 Elsevier Science Ltd.