Iron and phosphorus co-limit nitrogen fixation in the eastern tropical North Atlantic

Matthew M. Mills, Celine Ridame, Margaret Davey, Julie La Roche, Richard J. Geider

Résultat de recherche: Articleexamen par les pairs

774 Citations (Scopus)

Résumé

The role of iron in enhancing phytoplankton productivity in high nutrient, low chlorophyll oceanic regions was demonstrated first through iron-addition bioassay experiments and subsequently confirmed by large-scale iron fertilization experiments. Iron supply has been hypothesized to limit nitrogen fixation and hence oceanic primary productivity on geological timescales, providing an alternative to phosphorus as the ultimate limiting nutrient. Oceanographic observations have been interpreted both to confirm and refute this hypothesis, but direct experimental evidence is lacking. We conducted experiments to test this hypothesis during the Meteor 55 cruise to the tropical North Atlantic. This region is rich in diazotrophs and strongly impacted by Saharan dust input. Here we show that community primary productivity was nitrogen-limited, and that nitrogen fixation was co-limited by iron and phosphorus. Saharan dust addition stimulated nitrogen fixation, presumably by supplying both iron and phosphorus. Our results support the hypothesis that aeolian mineral dust deposition promotes nitrogen fixation in the eastern tropical North Atlantic.

Langue d'origineEnglish
Pages (de-à)292-294
Nombre de pages3
JournalNature
Volume429
Numéro de publication6989
DOI
Statut de publicationPublished - mai 20 2004
Publié à l'externeOui

Note bibliographique

Funding Information:
Acknowledgements We thank M. Thattai for stimulating discussions and helpful suggestions on measuring the escape rates; J. Pedraza, M. Kardar, O. Ozcan and S. Cabi for useful discussions; B. Kaufmann for help with image analysis; and B. Pando for comments on the manuscript. M.A. acknowledges support by an MIT Presidential Fellowship endowed by Praecis Pharmaceuticals, Inc. A.B. is a Long Term Fellow of the Human Frontiers Science Program. This work was supported by a NSF-CAREER and a NIH grant.

Funding Information:
Acknowledgements WewouldliketoacknowledgethecaptainandcrewoftheF/SMeteorandthe scientists aboard the Meteor 55 SOLAS cruise, especially D. Wallace, K. Lochte, H. Bange, P. Croot, M. Voss, F. Malien, R. Langlois and P. Fritsche. We thank D. Wallace for insightful comments on this manuscript. Additionally, we acknowledge W. Balzer for loaning the clean container used during M55. This work was supported by the Deutsche Forschungsgemeinschaft’s Meteor Schwerpunktprogramm, a Natural Environment Research Council grant to R.J.G., and a Marie Curie Post Doctoral fellowship to C.R.

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