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. Author manuscript; available in PMC: 2016 Jul 15.
Published in final edited form as: Meteorit Planet Sci. 2015 Jul 16;50(7):1197–1216. doi: 10.1111/maps.12461

Fig. 10.

Fig. 10

Pb-Pb ages versus initial 53Mn/55Mn for angrite, eucrite, and CB meteorites. Pb-Pb ages are from: Brennecka and Wadhwa (2012) for D’Orbigny, Angra dos Reis (hereafter “AdoR”) NWA 4801 and NWA 4590; Iizuka et al. (2014) for LEW 86010 and Ibitira; Connelly et al. (2008) U-corrected for Sahara 99555 (hereafter “SAH 99555”) and Connelly (personal communication) for NWA 1670 and NWA 2999; Zartman et al. (2006) U-corrected for Asuka 881371 (hereafter “A-881371”); this study for Gujba. Initial 53Mn/55Mn values are from: Glavin et al. (2004) for D’Orbigny, Sugiura et al. (2005) for Sahara, Asuka, and NWA 1670; Lugmair and Shukolyukov (1998) and Nyquist et al. (1994) for LEW and Ibitira; McKibbin et al. (2013) for AdoR; Shukolyukov et al. (2009) for NWA 4801; Shukolyukov and Lugmair (2008) for NWA 2999; Yin et al. (2009) for NWA 4590; Yamashita et al. (2010) for Gujba. Other values for D’Orbigny are from Nyquist et al. (2003), Sugiura et al. (2005), Yin et al. (2009) and McKibbin et al. (2013) as shown in the inserted plot. The two 53Mn decay lines are anchored to the initial 53Mn/55Mn for Gujba given by Yamashita et al. (2010) and for D’Orbigny given by Glavin et al. (2004).