Fig. 5: Comparison of lunar farside and nearside basalts and other basaltic meteorites.
From: Sulfur isotopes from the lunar farside reveal global volatile loss following the giant impact
Mare basalts show variable S content with high-Ti basalt higher than low-Ti basalts (a–c). The S/Dy of both low-Ti and high-Ti basalts are variable and lower than that of mid-ocean ridge basalts (212 ± 45)59 (d). The δ34S values further show a global homogeneity (0–1‰), although mantle domains are very heterogenous (e, f ). Data source: The δ34S values of meteorites (NWA 4734 and NWA 6950) are from the ref. 28. Ages of CE-6, CE-5, meteorites and Apollo basalts are from the refs. 24,32,33,73. The μ values (238U/204Pb ratio) of CE-6, CE-5, meteorites and Apollo basalts are from the literature33 and references therein.
