Molybdenum isotope anomalies in meteorites: Constraints on solar nebula evolution and origin of the Earth
By C. Burkhardt, T. Kleine, F. Oberli, A. Pack, B. Bourdon, R. Wieler. 2011
287 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Nuclear and High Energy Physics
View Paper: https://www.semanticscholar.org/paper/141943ef66cfb732cd729e23d9e6d82cb1015f92
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In Astronomy and Astrophysics
- A. Morbidelli
- Kevin J. Walsh
- C. Alexander
- F. DeMeo
- C. Burkhardt
- L. Elkins‐Tanton
- N. Dauphas
- Clark R. Chapman
In Nuclear and High Energy Physics
Citations in the corpus
- The Non-carbonaceous–Carbonaceous Meteorite Dichotomy (2020, background): “This includes enrichments in rprocess Mo (Brennecka et al. 2013; Burkhardt et al. 2011), 54Cr (Papanastassiou 1986), and coupled 46Ti–50Ti excesses (Davis et al. 2018; Trinquier et al. 2009).”
- Differentiated Planetesimals and the Parent Bodies of Chondrites (2013, background): “Over the past two decades, it has become clear that different meteorite groups also have distinct bulk isotopic compositions for a diversity of elements, including Cr, Ti, Mo, Ni, and Cu (e.g., Burkhardt et al. 2011).”
- Evidence for Mo isotope fractionation in the solar nebula and during planetary differentiation (2014, methodology): “Molybdenum was separated from the sample matrix using a three-stage ion exchange procedure employing both anion and cation exchange resins (Burkhardt et al., 2011).”
- Calcium-48 isotopic anomalies in bulk chondrites and achondrites: Evidence for a uniform isotopic reservoir in the inner protoplanetary disk (2014, background): “Also, molybdenum (Burkhardt et al., 2011) and titanium (Zhang et al., 2012) in enstatite chondrites may be slightly distinct from terrestrial composition – see Dauphas et al. (2002a) for an alternative view on molybdenum.”
- The Compositional Structure of the Asteroid Belt (2015, background): “There is clear isotopic evidence in O, Ti, Cr, Mo and Ru for a distinction between the carbonaceous chondrites and almost all other inner Solar System objects (including Earth, Moon and Mars) for which we have samples (Burkhardt et al., 2011; Warren, 2011).”
- Abundance, distribution, and origin of 60Fe in the solar protoplanetary disk (2012, background): “…phases, as had been documented previously for several other elements (Dauphas et al., 2002, 2004b; Hidaka et al., 2003; Andreasen and Sharma 2006, 2007; Trinquier et al., 2007, 2009; Carlson et al., 2007; Qin et al., 2008; Chen et al., 2010, 2011; Burkhardt et al., 2011; Moynier et al., 2012).”