53Mn–53Cr systematics of the early Solar System revisited

By A. Trinquier, J. Birck, C. Allègre, C. Göpel, D. Ulfbeck. 2008

247 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics, Ecology, Geophysics

View Paper: https://www.semanticscholar.org/paper/91887e67f008879d5b7ad99e4bba67727ed5f331

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Citations in the corpus

Chronology of the angrite parent body and implications for core formation in protoplanets (2012, background): “6 are two different estimates for the solar system initial 53Mn/55Mn: (6.3 ± 0.7) 10 6 as inferred from Mn–Cr data of inner solar system objects (Trinquier et al., 2008); and (9.1 ± 1.7) 10 6 as derived from a correlation of initial 26Al/27Al and 53Mn/55Mn ratios in meteorites (Nyquist et al. 2009).”
The Compositional Structure of the Asteroid Belt (2015, background): “t for details. b - Kleine et al., (2008). c - Harrison and Grimm (2010); Henke et al., (2013); Kleine et al., (2008); Trieloff et al., (2003). d - see text for details. e – Kleine et al., (2012). f - Trinquier et al., (2008). g - Schiller et al., (2011). h - Neumann et al., (2014). i - Kruijer et al”
HED Meteorites and Their Relationship to the Geology of Vesta and the Dawn Mission (2011, background): “The crystallization ages of basaltic eucrites indicate volcanism extended for ~10 Myr and possibly longer (Trinquier et al. 2008).”
The Effect of Jupiter's Formation on the Distribution of Refractory Elements and Inclusions in Meteorites (2017, unknown): “Chondrite parent bodies generally accreted later, with most OCs probably accreting 9 CI 3.6 ± 0.5a 4.4 − 5.7aa 3.1 - 4.1 a. Sugiura & Fujiya (2014); b. Melting event, Al-Mg: Baker et al. (2012); c. Impact event, Al-Mg and Hf-W: van Kooten et al. (2017); d. Wilson & Goodrich (2016); Goodrich et al. (”
Asteroid (4) Vesta: I. The howardite-eucrite-diogenite (HED) clan of meteorites (2015, background): “Trinquier et al. (2008) confirmed this absoute age for HED parent body differentiation, and pegged this event o 2.3 Myr after CAI formation.”
Abundance, distribution, and origin of 60Fe in the solar protoplanetary disk (2012, methodology): “This is consistent with the finding that Pasamonte and Ibitira also plot on the same bulk rock 53 Mn53 Cr (t1/2=3.74 Myr; Honda and Imamura, 1971) isochron as other eucrites (Lugmair and Shukolyukov, 1998; Trinquier et al., 2008).”