Stable calcium isotopic composition of meteorites and rocky planets
By J. Simon, D. DePaolo. 2010
165 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Ecology, Geophysics
View Paper: https://www.semanticscholar.org/paper/38a7f3bad06c991d16c05ea5c3fad38c0d42f0e1
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Citations in the corpus
- Evidence for Mo isotope fractionation in the solar nebula and during planetary differentiation (2014, background): “…1993), Zn, Cu, and Ni (Luck et al., 2005; Moynier et al., 2006), Cd (Wombacher et al., 2008), Cr (Moynier et al., 2011), Si (Armytage et al., 2011; Fitoussi et al., 2009; Savage and Moynier, 2013), Ca (Simon and DePaolo, 2010), and Sr (Charlier et al., 2012; Moynier et al., 2010; Patchett, 1980).”
- Heterogeneous accretion, composition and core–mantle differentiation of the Earth (2011, background): “Although primitivemeteorites are representative of early-accreted material, there is no single type of chondritic meteorite that would represent a suitable parental material for the Earth, neither with regard to chemistry nor isotopic composition (Drake and Righter, 2002; Simon and DePaolo, 2010; Tr”
- Calcium-48 isotopic anomalies in bulk chondrites and achondrites: Evidence for a uniform isotopic reservoir in the inner protoplanetary disk (2014, methodology): “, 2014) and against (Simon and DePaolo, 2010) a relationship between enstatite meteorites and Earth.”