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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 8054Achondrite-ung0.3720-1.5510-1.748-0.38 -0.11 0.09
GujbaCBa0.9800-1.7800-2.2960.23 -0.33 -0.46
Northwest Africa 8054Achondrite-ung0.3410-1.5990-1.779-0.41 -0.15 0.06
Sierra Gorda 013CBa0.6500-1.8890-2.232-0.1 -0.44 -0.39
Sierra Gorda 013CBa0.5900-1.9000-2.212-0.16 -0.45 -0.37
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