Terrestrial planet formation from lost inner solar system material-Reference-Cited by-同舟云学术

Terrestrial planet formation from lost inner solar system material

Published:2021-12-24 Issue:52 Volume:7 Page:
ISSN:2375-2548
Container-title:Science Advances
language:en
Short-container-title:Sci. Adv.

Author:

Burkhardt Christoph¹^ORCID,Spitzer Fridolin¹^ORCID,Morbidelli Alessandro²,Budde Gerrit³^ORCID,Render Jan H.¹^ORCID,Kruijer Thomas S.⁴⁵,Kleine Thorsten¹⁶^ORCID

Affiliation:

1. Institut für Planetologie, University of Münster, Wilhelm-Klemm-Str. 10, 48149 Münster, Germany.

2. Laboratoire Lagrange, UMR7293, Université de Nice Sophia-Antipolis, CNRS, Observatoire de la Côte d’Azur, Boulevard de l’Observatoire, 06304 Nice, Cedex 4, France.

3. Division of Geological and Planetary Sciences, California Institute of Technology, 1200 E California Blvd, Pasadena, CA 91125, USA.

4. Museum für Naturkunde, Leibniz Institute for Evolution and Biodiversity Science, Invalidenstraße 43, 10115 Berlin, Germany.

5. Institut für Geologische Wissenschaften, Freie Universität Berlin, Malteserstraße 74-100, 12249 Berlin, Germany.

6. Max Planck Institute for Solar System Research, Justus-von-Liebig-Weg 3, 37077 Göttingen, Germany.

Abstract

An integrated assessment of isotopic variations among meteorites reveals the process by which Earth and Mars are formed.

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

Reference62 articles.

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5. Growing the gas-giant planets by the gradual accumulation of pebbles

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