Changes in global nitrogen cycling during the Holocene epoch

Kendra K. McLauchlan, Joseph J. Williams, Joseph M. Craine, Elizabeth S. Jeffers

Research output: Contribution to journalArticlepeer-review

94 Scopus citations

Abstract

Human activities have doubled the pre-industrial supply of reactive nitrogen on Earth, and future rates of increase are expected to accelerate. Yet little is known about the capacity of the biosphere to buffer increased nitrogen influx. Past changes in global ecosystems following deglaciation at the end of the Pleistocene epoch provide an opportunity to understand better how nitrogen cycling in the terrestrial biosphere responded to changes in carbon cycling. We analysed published records of stable nitrogen isotopic values (δ 15 N) in sediments from 86 lakes on six continents. Here we show that the value of sedimentary δ 15 N declined from 15,000years before present to 7,056±597years before present, a period of increasing atmospheric carbon dioxide concentrations and terrestrial carbon accumulation. Comparison of the nitrogen isotope record with concomitant carbon accumulation on land and nitrous oxide in the atmosphere suggests millennia of declining nitrogen availability in terrestrial ecosystems during the Pleistocene-Holocene transition around 11,000 years before present. In contrast, we do not observe a consistent change in global sedimentary δ 15 N values during the past 500years, despite the potential effects of changing temperature and nitrogen influx from anthropogenic sources. We propose that the lack of a single response may indicate that modern increases in atmospheric carbon dioxide and net carbon sequestration in the biosphere have the potential to offset recent increased supplies of reactive nitrogen in some ecosystems.

Original languageEnglish (US)
Pages (from-to)352-355
Number of pages4
JournalNature
Volume495
Issue number7441
DOIs
StatePublished - Mar 21 2013

Bibliographical note

Funding Information:
Acknowledgements This work was supported by the National Science Foundation (BCS-0955225 and EPS-0903806) and a James Martin Fellowship at the University of Oxford. We thank the many authors who contributed their data for the purpose of this analysis. We appreciate technical assistance from C. Morris, P. Long and S. McConaghy. We thank J. Marlon, S. Enders, C. Baird and S. Perakis for comments.

Copyright:
Copyright 2013 Elsevier B.V., All rights reserved.

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