Enigmatic carbon isotopic variability in the oceanic upper mantle

Y Yves Moussallam (Lamont–Doherty Earth Observatory, Columbia University) E Estelle F. Rose-Koga (Institut des Sciences de la Terre d’Orléans, UMR 7327, Université Orléans–CNRS-Observatoire des Sciences de l'Univers en région Centre, 1A rue de la Férollerie) C Cyril Aubaud (Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, Laboratoire de Géochimie des Isotopes Stables) G Guillaume Georgeais (Lamont–Doherty Earth Observatory, Columbia University) P Pierre Cartigny (Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, Laboratoire de Géochimie des Isotopes Stables) K Kenneth T. Koga (Institut des Sciences de la Terre d’Orléans, UMR 7327, Université Orléans–CNRS-Observatoire des Sciences de l'Univers en région Centre, 1A rue de la Férollerie) J Jean-Luc Devidal (Laboratoire Magmas et Volcans, CNRS, Institut de Recherche pour le Développement, Observatoire de Physique du Globe de Clermont-Ferrand, Université Clermont Auvergne) P Peter J. Michael (School of Petroleum Engineering, The University of Tulsa) K Kei Shimizu A Alberto E. Saal (Department of Earth, Environmental and Planetary Sciences, Brown University)

Abstract

Unraveling the origin(s) of carbon on Earth has remained challenging, not only because of the multiple isotopic fractionation episodes that may have occurred during planet formation processes but also because the end point of these processes, the current isotopic value of Earth’s deep carbon reservoirs remains poorly constrained. Here, we present carbon isotopic measurements on rare undegassed mid-ocean ridge basalts from the Pacific, Atlantic, and Arctic Oceans that have preserved the isotopic signature of their mantle source. We find that Earth’s present-day convecting upper mantle has variable δ 13 C value from ~−10 to −4‰, significantly different from the δ 13 C value of peridotitic diamonds and with the highest values being restricted to the Atlantic. Evidence for significant mantle heterogeneity contrasts with previous assumptions and its origin remains puzzling being uncorrelated with geochemical markers associated with either subduction and surficial recycling processes or lower mantle contributions. The data do not preclude other causes such as primordial mantle heterogeneity. We suggest that the δ 13 C value of the bulk silicate Earth may need to be revised.

Article Details

Volume / Issue Vol. 122, Issue 25
Published June 24, 2025
ISSN 0027-8424
Publisher National Academy of Sciences

Authors (10)

Y

Yves Moussallam

Lamont–Doherty Earth Observatory, Columbia University

E

Estelle F. Rose-Koga

Institut des Sciences de la Terre d’Orléans, UMR 7327, Université Orléans–CNRS-Observatoire des Sciences de l'Univers en région Centre, 1A rue de la Férollerie

C

Cyril Aubaud

Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, Laboratoire de Géochimie des Isotopes Stables

G

Guillaume Georgeais

Lamont–Doherty Earth Observatory, Columbia University

P

Pierre Cartigny

Université Paris Cité, Institut de Physique du Globe de Paris, CNRS, Laboratoire de Géochimie des Isotopes Stables

K

Kenneth T. Koga

Institut des Sciences de la Terre d’Orléans, UMR 7327, Université Orléans–CNRS-Observatoire des Sciences de l'Univers en région Centre, 1A rue de la Férollerie

J

Jean-Luc Devidal

Laboratoire Magmas et Volcans, CNRS, Institut de Recherche pour le Développement, Observatoire de Physique du Globe de Clermont-Ferrand, Université Clermont Auvergne

P

Peter J. Michael

School of Petroleum Engineering, The University of Tulsa

K

Kei Shimizu

A

Alberto E. Saal

Department of Earth, Environmental and Planetary Sciences, Brown University