Research ArticlePLANETARY SCIENCE
Iron isotope evidence for very rapid accretion and differentiation of the proto-Earth
- View ORCID ProfileMartin Schiller1,*,
- View ORCID ProfileMartin Bizzarro1,2 and
- Julien Siebert2,3
- 1Centre for Star and Planet Formation, Globe Institute, University of Copenhagen, Øster Voldgade 5–7, DK-1350 Copenhagen, Denmark.
- 2Institut de Physique du Globe de Paris, Université Sorbonne Paris Cité, 75005 Paris, France.
- 3Institut Universitaire de France, Paris, France.
- ↵*Corresponding author. Email: schiller{at}ign.ku.dk
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Science Advances 12 Feb 2020:
Vol. 6, no. 7, eaay7604
DOI: 10.1126/sciadv.aay7604
Vol. 6, no. 7, eaay7604
DOI: 10.1126/sciadv.aay7604
Martin Schiller
1Centre for Star and Planet Formation, Globe Institute, University of Copenhagen, Øster Voldgade 5–7, DK-1350 Copenhagen, Denmark.
Martin Bizzarro
1Centre for Star and Planet Formation, Globe Institute, University of Copenhagen, Øster Voldgade 5–7, DK-1350 Copenhagen, Denmark.
2Institut de Physique du Globe de Paris, Université Sorbonne Paris Cité, 75005 Paris, France.
Julien Siebert
2Institut de Physique du Globe de Paris, Université Sorbonne Paris Cité, 75005 Paris, France.
3Institut Universitaire de France, Paris, France.
