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Oxygen isotope composition of Martian meteorites. Data for Martian meteorites from Franchi et al. (1999) and compiled from laser fluorination analyses in the Meteoritical Bulletin. MFL: Martian fractionation line of Franchi et al. (1999), TFL: terrestrial fractionation line.Δ17O calculated as: Δ17O = δ17O – 0.52δ18O. |
δ18O | δ17O | Δ17O: given | Δ17O: linear | Comment |
---|---|---|---|---|
7.2500 | 4.3600 | 0.5900 | 0.59 |
Name | Class | δ18O | δ17O | Δ17O: calc | Δ δ18O | Δ δ17O | Δ Δ17O |
---|---|---|---|---|---|---|---|
Northwest Africa 8114 | Martian (polymict breccia) | 7.2500 | 4.3600 | 0.59 | 0 | 0 | 0 |
Jiddat al Harasis 846 | OC3 | 7.2370 | 4.3960 | 0.633 | -0.01 | 0.04 | 0.04 |
Northwest Africa 8171 | Martian (polymict breccia) | 7.1800 | 4.4100 | 0.676 | -0.07 | 0.05 | 0.09 |
Hammadah al Hamra 180 | Chondrite-ung | 7.0700 | 4.4000 | 0.724 | -0.18 | 0.04 | 0.13 |
Jiddat al Harasis 846 | OC3 | 6.9990 | 4.2620 | 0.623 | -0.25 | -0.1 | 0.03 |
Loulan Yizhi 042 | H/L-melt rock | 6.8400 | 4.4390 | 0.882 | -0.41 | 0.08 | 0.29 |
Northwest Africa 12273 | Chondrite-ung | 7.2490 | 4.7860 | 1.017 | -0 | 0.43 | 0.43 |