The peridotites constituting the Earth's upper mantle are highly reactive when exposed to aqueous fluids under near-surface conditions (Kelemen & Hirth, 2012). Peridotite alteration is a major transfer process for volatiles between the hydrosphere and the lithosphere (Guillot & Hattori, 2013), and in the presence of carbon-bearing fluids it leads to carbonate precipitation (Power et al., 2013), which represents a natural mechanism for carbon capture and storage (Kelemen & Matter, 2008). Peridotite alteration is a complex process that can proceed along several different chemical reaction paths depending on the details of the fluid and rock compositions. These reaction paths have been described (e.g., Johannes, 1969;B. W. Evans, 1977;Frost, 1985), but the physical processes associated with peridotite alteration, including how fluids migrate in the rock, how fluids penetrate into fresh rock and generate complex vein networks (Aupart et al., 2021;Iyer et al., 2008), and how these processes are affected by variations in reaction chemistry, are poorly understood.