Silicon isotopes in meteorites and planetary core formation

By R. Armytage, R. B. Georg, P. Savage, H. Williams, A. Halliday. 2011

134 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Atmospheric Science

View Paper: https://www.semanticscholar.org/paper/348df26e8ad9b1ab51ca6d2d4393a28f2eae0dc4

How researchers see this paper

The researchers whose trusted networks rank it highest, strongest advocate first. Every researcher gets a different order.

In Astronomy and Astrophysics

1. C. Burkhardt
2. T. Kleine
3. N. Dauphas
4. B. Bourdon
5. R. Hin
6. H. Kobayashi
7. A. Morbidelli
8. E. Scott

In Atmospheric Science

1. N. Dauphas
2. C. Burkhardt
3. T. Kleine
4. B. Bourdon

Citations in the corpus

• Evidence for Mo isotope fractionation in the solar nebula and during planetary differentiation (2014, background): “…of the bulk silicate Earth are fractionated compared to primitive meteorites, and this has been interpreted to indicate Si and Cr partitioning into the Earth’s core (Armytage et al., 2011; Fitoussi et al., 2009; Georg et al., 2007; Hin et al., 2014; Moynier et al., 2011; Shahar et al., 2011).”
• Planetary and meteoritic Mg/Si and δ30Si variations inherited from solar nebula chemistry (2015, background): “However, basalts have δ(30)Si values indistinguishable from mantle peridotites, suggesting that basalts are representative of their mantle source (Fitoussi et al., 2009; Savage et al., 2010; Savage et al., 2011; Armytage et al., 2011; Zambardi and Poitrasson, 2011; Savage and Moynier, 2013; Zambardi”