Pressure fundamentally influences these processes and is a necessary parameter to know for many of the models and tools we use to describe and investigate them (e.g., Jupp & Schultz, 2004;Monecke et al., 2014). Despite this necessity, few methods are available for estimating paleodepths of seawater in ancient, open ocean volcanic terranes (Monecke et al., 2014). This paper aims to present an improved paleobathymetric approach for ancient seafloor lava eruptions and to apply it to the archetypal Samail (Oman-UAE) and Troodos (Cyprus) ophiolites.For submarine volcanic terranes that accumulated below storm wave base, the three most promising lines of paleobathymetric evidence are the sedimentary record (e.g., pelagic carbonates indicating depths shallower than the carbonate compensation depth (CCD); Robertson, 2004), fluid inclusion evidence (e.g., in inclusions trapped in minerals formed at the seafloor; Spooner, 1980), and the concentrations of volatiles dissolved in volcanic glasses, which are partly dependent on pressure during quenching (Roberge et al., 2005). In the following, we determine the dissolved H 2 O concentrations and maximum permissible CO 2 concentrations of volcanic glasses from the Samail ophiolite, and interpret these in terms of paleodepths of eruption together with a similar, recently published data set from the Troodos ophiolite (Woelki et al., 2020). We then compare these predictions to sedimentary and fluid inclusion evidence from both ophiolites, finding