Nickel isotope heterogeneity in the early Solar System
By M. Regelous, T. Elliott, C. Coath. 2008
200 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Ecology, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/0a847823873d2707ae1185cf855f1443fcd5ce16
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Citations in the corpus
- Calcium-48 isotopic anomalies in bulk chondrites and achondrites: Evidence for a uniform isotopic reservoir in the inner protoplanetary disk (2014, background): “…groups formed from the same isotopic reservoir (O: Clayton et al., 1984; Ti: Trinquier et al., 2009; Zhang et al., 2012; Cr: Trinquier et al., 2007; Qin et al., 2010; Ni: Steele et al., 2012; Tang and Dauphas, 2012; Regelous et al., 2008; Mo: Dauphas et al., 2002a; Burkhardt et al., 2011).”
- Molybdenum isotope anomalies in meteorites: Constraints on solar nebula evolution and origin of the Earth (2011, background): “…and planetary scale has been observed for a number of elements, including Ti (Trinquier et al., 2007), Cr (Qin et al., 2010; Trinquier et al., 2009), Ni (Regelous et al., 2008), Mo (Dauphas et al., 2002b), Ru (Chen et al., 2010), Ba, Nd and Sm (Andreasen and Sharma, 2007; Carlson et al., 2007).”
- Hf–W mineral isochron for Ca,Al-rich inclusions: Age of the solar system and the timing of core formation in planetesimals (2008, background): “However, two more recent studies showed that there are no 60Ni deficits in iron meteorites and argue against a late injection of 60Fe (Dauphas et al., 2008; Regelous et al., 2008).”
- Stable-isotopic anomalies and the accretionary assemblage of the Earth and Mars: A subordinate role for carbonaceous chondrites (2011, methodology): “3; cf. analogous diagrams, based on smaller data sets, in Bizzarro et al., 2007; Regelous et al., 2008; however, as mentioned previously, the ε62Ni data of Bizzarro et al. are not used in this work).”
- The Non-carbonaceous–Carbonaceous Meteorite Dichotomy (2020, background): “…anomalies have now been identified for many elements, and it has been shown that they exist not only in bulk carbonaceous chondrites, but also in other groups of meteorites (e.g., Burkhardt et al. 2011; Dauphas et al. 2002; Leya et al. 2008; Regelous et al. 2008; Trinquier et al. 2007, 2009).”
- Abundance, distribution, and origin of 60Fe in the solar protoplanetary disk (2012, background): “A difficulty with ε 60 Ni is that different chondrite groups have different ε 60 Ni, ε 62 Ni, and ε 64 Ni values that partly correlate with isotopic anomalies in 54 Cr (Dauphas et al., 2008; Regelous et al., 2008; Tang and Dauphas, 2010; Warren 2011; Steele et al., 2012).”