Spatial distribution of isotopes and compositional mixing in the inner protoplanetary disk

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Table A.1

Mass-independent isotopic variations among the noncarbonaceous meteorite parent bodies.

		∆¹⁷O	2sd	References	ε⁵⁴Cr	2se	References
NC chondrites	H	0.73	0.18	1	−0.36	0.10	17, 18, 19
	L	1.07	0.18	1	−0.36	0.08	17, 18, 20
	LL	1.26	0.24	1	−0.43	0.05	17, 18
	EH	−0.02	0.34	1	0.04	0.05	17, 18, 21, 22, 23
	EL	0.00	0.13	1	0.04	0.05	17, 18, 21
	Rumuruti chondrites	2.72	0.62	2	−0.06	0.02	24, 25

Planetary bodies	Mars	0.32	0.03	1	−0.16	0.03	17, 18, 26
	Earth	0.007	0.012	3	0.08	0.02	7, 17, 18, 19, 21, 25, 27, 28, 29, 30, 31
	Moon	0.010	0.012	3	0.13	0.09	18, 21

Parent bodies of NC primitive achondrites	Acapulcoites-Lodranites	−1.12	0.36	1	−0.58	0.09	11, 20, 24, 32
	Brachinites	−0.25	0.18	1	−0.46	0.16	33
	Winonaites	−0.51	0.08	1	−0.52	0.06	20, 32
	Ureilites	−0.96	1.00	1	−0.91	0.04	24, 30, 32, 34, 35, 36, 37

Parent bodies of NC magmatic achondrites and stony-iron meteorites	Vesta (HED meteorites -mesosiderites)	−0.24	0.02	1	−0.69	0.06	17, 18
	Angrites	−0.072	0.014	1	−0.43	0.05	17, 19, 24, 28, 38
	Aubrites (main-group)	0.012	0.014	1	0.07	0.06	17, 31
	Shallowater	−0.02	0.04	4	−0.12	0.04	31
	NWA 5363 / 5400	0.00	0.07	5, 6, 7	−0.32	0.06	7, 39
	NWA 8054	−1.76	0.04	8	−0.44	0.08	33
	NWA 7325	−0.76	0.15	9, 10, 11	−0.57	0.06	11, 40
	Ibitira	−0.065	0.014	12, 13	−0.40	0.08	41
	Asuka 881394, Bunburra	−0.13	0.05	1, 13	−0.40	0.06	42, 43, 44
	Rockhole, Emmaville,
	Dho 007, EET 92023
	Pasamonte, PCA 91007	−0.204	0.011	1, 13	−0.28	0.12	41
	NWA 1240	−0.271	0.014	13	−0.63	0.10	41
	NWA 11042/4284	1.02	0.04	1, 14	−0.29	0.08	14
	LEW 88763	−1.19	0.02	15
	NWA 2353 / 2635	0.54	0.27	5
	NWA 2993	−0.19	0.03	5
	NWA 5297 / 6698	1.21	0.08	5
	NWA 5517	−0.90	0.02	5
	NWA 11916	−0.45	0.03	5
	Pallasites (Krasnojarsk)	−0.18	0.04	16	−0.72	0.10	17
	Pallasites (Brenham)	−0.19	0.05	16	−0.06	0.11	18

References. (1) Greenwood et al. (2017); (2) Bischoff et al. (2011); (3) Greenwood et al. (2018); (4) Newton et al. (2000); (5) Meteoritical Bulletin Database (https://www.lpi.usra.edu/meteor/metbull.php); (6) Day et al. (2012); (7) Burkhardt et al. (2017); (8) Irving et al. (2014); (9) Barrat et al. (2015); (10) Weber et al. (2016); (11) Goodrich et al. (2017); (12) Wiechert et al. (2004); (13) Scott et al. (2009); (14) Váci et al. (2020); (15) Greenwood et al. (2012); (16) Greenwood et al. (2006); (17) Trinquier et al. (2007); (18) Qin et al. (2010a); (19) Schiller et al. (2014); (20) Schmitz et al. (2016); (21) Mougel et al. (2018); (22) Zhu et al. (2020a); (23) Zhu et al. (2021b); (24) Larsen et al. (2011); (25) Zhu et al. (2021a); (26) Kruijer et al. (2020); (27) van Kooten et al. (2016); (28) Zhu et al. (2019); (29) van Kooten et al. (2020); (30) Zhu et al. (2020b); (31) Zhu et al. (2021c); (32) Li et al. (2018); (33) Williams et al. (2020); (34) Shukolyukov & Lugmair (2006); (35) Ueda et al. (2006); (36) Qin et al. (2010b); (37) Yamakawa et al. (2010); (38) Shukolyukov et al. (2009); (39) Sanborn et al. (2016b); (40) Sanborn et al. (2013); (41) Sanborn & Yin (2014); (42) Sanborn et al. (2016a); (43) Benedix et al. (2017); (44) Wimpenny et al. (2019).

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