Organic carbon burial and degradation in marine sediments is an important factor in the regulation of Earth's climate on geologic time scales (LaRowe et al., 2020) and has been suggested as a possible carbon sink, which can explain observed decreases in atmospheric CO 2 over the past 50 million years (IPCC, 2021). Therefore, quantifying the amount and spatial distribution of organic carbon sequestered in marine sediments is fundamental to understanding global carbon cycling associated with climate variability via source and sink carbon interactions with the biosphere. Organic carbon is initially deposited on the seafloor through the outflow of terrestrial sources (i.e., rivers) and/or sinking of dead and decaying organisms (e.g., marine snow). Over time, this pool of shallow organic carbon deposited at the seafloor is either oxidized or buried where it can undergo a series of microbially driven redox reactions ultimately rendering methane (CH 4 ) (Middelburg, 2019). The majority of methane found in the subsurface is hypothesized to be of microbial origin (Kvenvolden, 1995), but abiotic thermogenic reactions also occur (Etiope & Sherwood Lollar, 2013).Methane produced in the subsurface is commonly incorporated into one of the largest estimated free carbon pools on Earth, methane hydrate (Ruppel & Kessler, 2017). Methane at a concentration level that exceeds local solubility and occurs within a specific pressure-temperature regime, referred to herein as the hydrate stability zone (HSZ), may form methane hydrates. The carbon sequestered in this ice-like substance is estimated to comprise ∼15%-50% of all global free carbon (Ruppel & Kessler, 2017). The HSZ generally occurs in water depths >300 m below sea level (mbsl), where pressures are high (∼3-30 MPa) and seafloor temperatures are low (<25°C) (Max et al., 2006;Ruppel & Waite, 2020). The thickness of the HSZ is controlled by the temperature, pressure, and salinity gradients in the subseafloor. Direct, global subseafloor observations of the HSZ are sparse, therefore the identification of the HSZ is first-order dependent upon accurate estimates of input parameters such as pressure, temperature, and geothermal gradient.