A plume origin for hydrous melt at the lithosphere–asthenosphere boundary

Plate tectonics requires a low-viscosity layer beneath the lithosphere–asthenosphere boundary (LAB), yet the origin of this ductile transition remains debated 1 , 2 . Explanations include the weakening effects of increasing temperature 3 , 4 , mineral hydration 5 or partial melt 6 . Electrical resistivity is sensitive to all three effects 7 , including melt volatile content 8 , but previous LAB constraints from magnetotelluric soundings did not simultaneously consider the thermodynamic stability of the inferred amount of melt and the effect of uncertainty in the estimated resistivity 8 – 14 . Here we couple an experimentally constrained parameterization of mantle melting in the presence of volatiles 15 , 16 with Bayesian resistivity inversion 17 and apply this to magnetotelluric data sensitive to a LAB channel beneath the Cocos Plate 9 . Paradoxically, we find that the conductive channel requires either anomalously large melt fractions with moderate volatile contents or moderate melt fractions with anomalously large volatile contents, depending on the assumed mantle temperature. Large melt fractions are unlikely to be mechanically stable and conflict with melt-migration models 18 . As large volatile contents require a highly enriched mantle source inconsistent with mid-ocean-ridge estimates 19 , our results indicate that a mantle plume emplaced volatile-rich melts in the LAB channel. This requires the presence of a previously undetected nearby plume or the influence of the distant Galápagos hotspot. Plumes that feed thin, hydrous melt channels 9 , 14 , 20 may be an unrecognized source of LAB anomalies globally. By combining experimental constraints on mantle melting with magnetotelluric data, volatile-rich melts emplaced by a mantle plume were shown to be present in the asthenosphere beneath the Cocos Plate.