Manganese–chromium isotope systematics of carbonaceous chondrites

By A. Shukolyukov, G. W. Lugmair. 2006

147 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Geophysics

View Paper: https://www.semanticscholar.org/paper/f48ceac8c4a5c1dfa8624a510b35c9ce0b1c35c9

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In Astronomy and Astrophysics

1. P. Warren
2. A. Krot
3. H. Palme
4. I. Franchi
5. F. Moynier
6. T. Burbine
7. R. Greenwood
8. M. F. Miller

In Geophysics

1. F. Moynier
2. I. Franchi
3. T. Burbine
4. R. Greenwood
5. M. F. Miller
6. P. Warren
7. Q. Yin
8. A. Krot

Citations in the corpus

• 26 Al- 26 Mg and 207 Pb- 206 Pb systematics of Allende CAIs: Canonical solar initial 26 Al/ 27 Al ratio reinstated (2008, methodology): “…have also measured 55Mn/52Crwith similarmethod (Moynier et al., 2007), and comparedour determinations to the measurements by ICP-OES (optical emission spectrometry, an analytical method different from mass spectrometry) performed by Shukolyukov and Lugmair (2006) on various carbonaceous chondrites.”
• Calcium-48 isotopic anomalies in bulk chondrites and achondrites: Evidence for a uniform isotopic reservoir in the inner protoplanetary disk (2014, unknown): “…iron-peak elements, such as 48Ca (H.-W. Chen et al., 2011), 50Ti (Niederer et al., 1985b; Niemeyer, 1985, 1988; Trinquier et al., 2009; Zhang et al., 2011, 2012), 54Cr (Shukolyukov and Lugmair, 2006; Trinquier et al., 2007; Qin et al., 2010), and 64Ni (Steele et al., 2011; Tang and Dauphas, 2014).”
• Melting and differentiation of early-formed asteroids: The perspective from high precision oxygen isotope studies (2017, background): “It was pointed out by Warren (2011a,b), based on data from earlier studies (e.g. Shukolyukov and Lugmair, 2006; Trinquier et al., 2007, 2009; Qin et al., 2010a,b), that Solar System materials display a bimodal distribution with respect to a range of stable nuclides, including 54Cr, 50Ti and 62Ni.”
• Nickel isotope heterogeneity in the early Solar System (2008, background): “Stepwise leaching of CI chondrites has shown that neutron-rich (54)Cr (and by implication (62)Ni) is apparently carried in a more widely dispersed silicate phase in the least metamorphosed carbonaceous chondrite types (Rotaru et al., 1992; Shukolyukov and Lugmair, 2006; Trinquier et al., 2007), and ”
• NEUTRON-RICH CHROMIUM ISOTOPE ANOMALIES IN SUPERNOVA NANOPARTICLES (2010, background): “…to be the sole carriers of the 54Cr anomalies measured in this sample and perhaps in planetary materials, in general (Rotaru et al. 1992; Podosek et al. 1997, 1999; Nichols et al. 1998, 2000; Alexander 2002; Shukolyukov & Lugmair 2006; Trinquier et al. 2007; Birck et al. 2009; Qin et al. 2010).”
• Stable-isotopic anomalies and the accretionary assemblage of the Earth and Mars: A subordinate role for carbonaceous chondrites (2011, background): “2, the Eagle Station pallasites (actually only “ES” itself has thus far been analyzed: Shukolyukov and Lugmair, 2006b) plot far from all other metal-rich differentiated materials, yet not at a randomposition; they plotwithin the narrowcarbonaceous field. Humayun and Weiss (2011) found that siderophi”