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Meteoritical Bulletin: Oxygen Isotope Plots

Change plot type:
Change values (separate multiple values with semicolons) -    δ18O:    δ17O:    Δ17O:
Change title:

Oxygen isotope composition of differentiated achondrites. Data for angrites and HEDs from Greenwood et al. (2005). Data for Martian meteorites from Franchi et al. (1999). EFL: eucrite fractionation line (Greenwood et al., 2005), AFL: angrite fractionation line (Greenwood et al., 2005), MFL: Martian fractionation line (Franchi et al., 1999), TFL: terrestrial fractionation line. M: average value of Martian meteorite analyses from Franchi et al. (1999). E: bulk terrestrial mantle (Mattey et al., 1994). Open squares: HEDs, open triangles: angrites, open circles: Martian meteorites. Δ17O is linearized using the format of Miller (2002): Δ17O = 1000 ln (1+ (δ17O/1000)) – λ1000 ln (1+ ( δ18O/1000)) where λ = 0.5247.


Data summary:
δ18Oδ17OΔ17O: givenΔ17O: Miller (2002)Comment

Nearest neighbors in MBDB (within 0.5 permil):
NameClassδ18Oδ17OΔ17O: calcΔ δ18OΔ δ17OΔ Δ17O
Northwest Africa 12969Achondrite-ung6.28001.5010-1.7880.04 0.02 -0
Northwest Africa 11187Achondrite-ung6.19801.5440-1.702-0.04 0.06 0.09
Northwest Africa 11187Achondrite-ung6.31801.5810-1.7280.08 0.1 0.06
Northwest Africa 11511Ureilite-an6.12801.6220-1.588-0.11 0.14 0.2
Northwest Africa 12969Achondrite-ung6.06401.3540-1.822-0.18 -0.13 -0.03
Northwest Africa 11187Achondrite-ung6.00301.4500-1.694-0.24 -0.03 0.09
Northwest Africa 10324CR25.95001.7900-1.327-0.29 0.31 0.46
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