Iron isotope evidence for very rapid accretion and differentiation of the proto-Earth-Reference-Cited by-同舟云学术

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Iron isotope evidence for very rapid accretion and differentiation of the proto-Earth

Published:2020-02-14 Issue:7 Volume:6 Page:
ISSN:2375-2548
Container-title:Science Advances
language:en
Short-container-title:Sci. Adv.

Author:

Schiller Martin¹^ORCID,Bizzarro Martin¹²^ORCID,Siebert Julien²³

Affiliation:

1. Centre for Star and Planet Formation, Globe Institute, University of Copenhagen, Øster Voldgade 5–7, DK-1350 Copenhagen, Denmark.

2. Institut de Physique du Globe de Paris, Université Sorbonne Paris Cité, 75005 Paris, France.

3. Institut Universitaire de France, Paris, France.

Abstract

The iron isotope composition of Earth’s mantle requires planetary growth within 5 Ma of solar system formation.

Funder

H2020 European Research Council

Danish National Research Foundation

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference57 articles.

1. Growth of asteroids, planetary embryos, and Kuiper belt objects by chondrule accretion

2. A low mass for Mars from Jupiter’s early gas-driven migration

3. The cometary contribution to the oceans of primitive Earth

4. Source regions and timescales for the delivery of water to the Earth

5. The Delivery of Water During Terrestrial Planet Formation

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