Ferrovolcanism on metal worlds and the origin of pallasites
Brandon C. Johnson, Michael M. Sori, Alexander J. Evans

TL;DR
This paper explores ferrovolcanism, a process where sulfur-enriched FeNi melts intrude or erupt on metal-rich planetary bodies, potentially explaining the origin of pallasite meteorites and surface features of bodies like Psyche.
Contribution
It introduces the concept of ferrovolcanism driven by residual sulfur-enriched FeNi melts and links this process to the formation of pallasites and surface phenomena on metal worlds.
Findings
Ferrovolcanic eruptions are more likely on bodies with mantles less than 50 km thick.
Residual sulfur-enriched FeNi melts can propagate into the mantle via dikes.
Ferrovolcanism may explain the metallic surface of Psyche despite its bulk density.
Abstract
As differentiated planetesimals cool, their cores can solidify from the outside-in, as evidenced by paleomagnetic measurements and cooling rate estimates of iron meteorites. The details of outside-in solidification and fate of residual core melt are poorly understood. For a core primarily composed of Fe and Ni alloyed with lighter constituent elements, like sulfur, such inward core growth would likely be achieved by growth of solid FeNi dendrites. Growth of FeNi dendrites results in interconnected pockets of residual melt that become progressively enriched in sulfur up to a eutectic composition of 31 wt percent sulfur as FeNi continues to solidify. Here we show that regions of residual sulfur-enriched FeNi melt in the core attain sufficient excess pressures to propagate via dikes into the mantle. Thus, core material will intrude into the overlying rocky mantle or possibly even erupt…
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