Ammonia-water freezing as a mechanism for recent cryovolcanism on Pluto

Abstract NASA's New Horizons flyby of the Pluto-Charon system in 2015 exposed a multitude of geologically active terrains on the surface of Pluto. Possible evidence of cryovolcanism has been reported in association with crustal scale extensional tectonic structures at Virgil Fossae and at two large circular mountains, informally referred to as Wright Mons and Piccard Mons. Our detailed geologic mapping of Wright Mons and the surrounding region reveals additional circular mounds overlying the main edifice and narrow ravines emanating from the summit, possibly produced by liquid flow. We model the overpressure generated during the freezing of a mixed ammonia-water liquid inside an enclosed chamber in Pluto's ice crust and in a global subsurface ocean. We consider scenarios spanning the possible range of Pluto's ammonia abundance and conclude that stresses generated due to freezing-induced pressurization can exceed the tensile strength of ice and create fractures for the liquid to escape. Our results suggest that freezing in a crustal chamber and the subsurface ocean are both viable mechanisms for cryovolcanism on Pluto and may explain the morphological variety of cryovolcanic formations observed by New Horizons.