Summary: | The Powai ankaramite flow from Mumbai, western Deccan Traps, contains abundant crystals of augite (En[subscript 59–47]Fs[subscript 10–14]Wo[subscript 27–42], 22–40 modal %, 3–5 mm) and olivine (Fo[subscript 84–74], 11–16 modal %, 1–2 mm), and minor plagioclase (An[subscript 71], ~0.5 mm) embedded in a fine-grained matrix. Minor orthopyroxene (En[subscript 79–77]Fs[subscript 16–19]Wo[subscript 5–4]) with irregular and embayed margins is mantled by thick augite overgrowth rims. The Fe–Mg distribution between the large crystals and bulk rock shows disequilibrium, indicating that the ankaramite is a cumulate rock. The ankaramite probably formed by the intrusion of tholeiitic melt into a cumulate pile with olivine, augite, and orthopyroxene left by the crystallization of earlier magmas, resulting in orthopyroxene dissolution and subsequent precipitation of augite. Olivine-hosted melt inclusions and melts represented by the ankaramite groundmass and some associated tholeiitic dikes are multiply saturated with olivine + plagioclase + clinopyroxene at ≤6 kb according to phase equilibrium constraints. Calculations involving incremental addition of equilibrium phases to these melts and to the common aphyric tholeiites of the voluminous Ambenali and Mahabaleshwar Formations show that their primary magmas (wt% SiO[subscript 2]: 48–50, MgO: 9.8–11.8, and FeO: 7.2–7.9, and Mg# 70–74) last equilibrated with spinel lherzolite at ~8–13 kb (~30–49 km depths) and ~1268–1332 °C, and trace element considerations indicate ≤15 % batch melting of mantle. These tholeiitic primary magmas then underwent olivine gabbro fractionation in upper crustal magma chambers at depths ≤23 km. The minimum depth of equilibration of the primary magmas is shallower than the present-day Moho in the Mumbai area based on seismological data, indicating localized mantle upwelling and lower crustal interactions previously inferred from the Nd–Sr isotopic ratios and other geochemical characteristics of the ankaramite and associated tholeiites.
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