Earth’s water may have been inherited from material similar to enstatite chondrite meteorites

Author:

Piani Laurette1ORCID,Marrocchi Yves1ORCID,Rigaudier Thomas1ORCID,Vacher Lionel G.12,Thomassin Dorian1,Marty Bernard1ORCID

Affiliation:

1. Centre de Recherches Pétrographiques et Géochimiques (CRPG), Centre National de Recherche Scientifique (CNRS)–Université de Lorraine, Vandoeuvre-les-Nancy, F-54500, France.

2. Department of Physics, Washington University in St. Louis, St. Louis, MO 63130, USA.

Abstract

An unexpected source of Earth's water The abundances of Earth's chemical elements and their isotopic ratios can indicate which materials formed Earth. Enstatite chondrite (EC) meteorites provide a good isotopic match for many elements but are expected to contain no water because they formed in the hot inner Solar System. This would require Earth's water to be from a different source, such as comets. Piani et al. measured hydrogen contents and deuterium/hydrogen ratios (D/H) in 13 EC meteorites (see the Perspective by Peslier). They found far more hydrogen than is commonly assumed, with D/H close to that of Earth's mantle. Combining these data with cosmochemical models, they show that most of Earth's water could have formed from hydrogen delivered by EC meteorites. Science , this issue p. 1110 ; see also p. 1058

Funder

European Research Council

Agence Nationale de la Recherche

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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