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Cited by 114Astro and Planetary ScienceGeological and Geochemical AnalysisPaleontology and Stratigraphy of Fossils

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The W isotope evolution of the bulk silicate Earth: constraints on the timing and mechanisms of core formation and accretion

Kleine, T., Mezger, K., Palme, H., Münker, C.·2004·Earth and Planetary Science Letters
DOI 10.1016/j.epsl.2004.09.023
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    “Thus, the formation of Earth commenced no earlier than 10 million years after the formation of the Solar System (Kleine et al., 2004; Jacobsen, 2005; Touboul et al., 2007).”

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Metadata

Authors
Kleine, T., Mezger, K., Palme, H., & Münker, C.
Affiliations
  • University of Münster (DE)
  • University of Cologne (DE)
Corresponding author
Kleine, T.
ORCID
Venue
Earth and Planetary Science Letters
Publisher
Elsevier BV
Published
2004-11
Volume
228
Issue
1-2
Pages
109-123
ISSN
0012-821X (ISSN-L)
DOI
10.1016/j.epsl.2004.09.023
OpenAlex
W2003563858
Cited by
114
References
1
Citations by year
2026: 2 · 2025: 4 · 2024: 3 · 2023: 2 · 2022: 3 · 2021: 4 · 2020: 5 · 2019: 2 · 2018: 4 · 2017: 6 · 2016: 5 · 2015: 6 · 2014: 5 · 2013: 2 · 2012: 4
FWCI
4.52
Type
journal article
Language
en
Open access
closed
Licence
www.elsevier.com/tdm/userlicense/1.0/ (tdm)
Locations
  • Earth and Planetary Science Letters (publishedVersion)
  • Bern Open Repository and Information System (University of Bern) (submittedVersion)
Funders
Deutsche Forschungsgemeinschaft
Topics
  • Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
  • Physical Sciences › Earth and Planetary Sciences › Geochemistry and Petrology › Geological and Geochemical Analysis
  • Physical Sciences › Earth and Planetary Sciences › Paleontology › Paleontology and Stratigraphy of Fossils
Keywords
tungsten isotopes, bulk silicate Earth, core formation, Earth accretion, metal-silicate equilibration, Moon-forming impact, Hf isotopes, chondrites

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