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. Author manuscript; available in PMC: 2021 Jul 26.
Published in final edited form as: Geochim Cosmochim Acta. 2021 Mar 10;301:70–90. doi: 10.1016/j.gca.2021.03.004

Fig. 8.

Fig. 8.

Plots of (A) Δ17O versus ε50Ti and (B) Δ17O versus ε54Cr for bulk carbonaceous chondrite samples studied here and from the literature. The ε50Ti and ε54Cr data for Coolidge, EET 83226, EET 83355, NWA 5958, MAC 87300, MAC 87301, MAC 88107, LEW 85332, and GRO 95566 are from this study, as are the Δ17O data for each of these samples except GRO 95566 (Clayton and Mayeda, 1999) and NWA 5958 (Jacquet et al., 2016). The Δ17O, ε50Ti, and ε54Cr data for individual CM, CO, CV, CK, CR, CB, and CI chondrites measured previously are from: (1) Shukolyukov and Lugmair (2006); (2) Trinquier et al. (2007); (3) Trinquier et al. (2009); (4) Qin et al. (2010); (5) Yamashita et al. (2010); (6) Zhang et al. (2011); (7) Zhang et al. (2012); (8) Sanborn et al. (2019); (9) Weisberg et al. (1993); (10) Clayton and Mayeda (1999); (11) Greenwood and Franchi (2004); (12) Greenwood et al. (2010); (13) Schrader et al. (2011); (14) Hewins et al. (2014); (15) Jacquet et al. (2016); and (16) Williams et al. (2020), as denoted by the numbers in parentheses in the legend. Error bars are internal 2SE or external 2SD, whichever is larger.