1Michael W. Broadley,2Peter H. Barry,1David V. Bekaert,1David J. Byrne,3Antonio Caracausi,4Christopher J. Ballentine,1Bernard Marty
Proceedings of the National Academy of Sciences of the Unites States of America (in Press) Link to Article [https://doi.org/10.1073/pnas.200390711]
1Centre de Recherches Pétrographiques et Géochimiques, UMR 7358 CNRS—Université de Lorraine, BP 20, F-54501 Vandoeuvre-lès-Nancy, France;
2Marine Chemistry and Geochemistry Department, Woods Hole Oceanographic Institution, Woods Hole, MA 02543;
3Instituto Nazionale di Geofisica e Vulcanologia, 90146 Palermo, Italy;
4Department of Earth Sciences, University of Oxford, OX1 3AN Oxford, United Kingdom
Identifying the origin of noble gases in Earth’s mantle can provide crucial constraints on the source and timing of volatile (C, N, H2O, noble gases, etc.) delivery to Earth. It remains unclear whether the early Earth was able to directly capture and retain volatiles throughout accretion or whether it accreted anhydrously and subsequently acquired volatiles through later additions of chondritic material. Here, we report high-precision noble gas isotopic data from volcanic gases emanating from, in and around, the Yellowstone caldera (Wyoming, United States). We show that the He and Ne isotopic and elemental signatures of the Yellowstone gas requires an input from an undegassed mantle plume. Coupled with the distinct ratio of 129Xe to primordial Xe isotopes in Yellowstone compared with mid-ocean ridge basalt (MORB) samples, this confirms that the deep plume and shallow MORB mantles have remained distinct from one another for the majority of Earth’s history. Krypton and xenon isotopes in the Yellowstone mantle plume are found to be chondritic in origin, similar to the MORB source mantle. This is in contrast with the origin of neon in the mantle, which exhibits an isotopic dichotomy between solar plume and chondritic MORB mantle sources. The co-occurrence of solar and chondritic noble gases in the deep mantle is thought to reflect the heterogeneous nature of Earth’s volatile accretion during the lifetime of the protosolar nebula. It notably implies that the Earth was able to retain its chondritic volatiles since its earliest stages of accretion, and not only through late additions.