“…Second, it has been proposed that formation of carbonate minerals via reaction of surface waters with peridotite can produce a significant carbon reservoir on this and other planets, and could potentially be emulated in accelerated systems for engineered carbon capture and storage (e.g., Kelemen & Matter, 2008). There have been numerous, related studies of carbon mineralization during natural weathering of peridotite in the Samail ophiolite (Chavagnac, Ceuleneer, et al., 2013; Chavagnac, Monnin, et al., 2013; Falk et al., 2016; Giampouras et al., 2020; Kelemen et al., 2011; Lacinska et al., 2014; Lacinska & Styles, 2013; Leleu et al., 2016; Mervine et al., 2014, 2015; Noël et al., 2018; Paukert Vankeuren et al., 2012, 2019; Rajendran et al., 2014; Rajendran & Nasir, 2019; Streit et al., 2012), elsewhere on Earth (e.g., Alt et al., 2012, 2013; Andrews et al., 2018; Arcilla et al., 2011; Beinlich et al., 2010; del Real et al., 2016; Gahlan et al., 2020; Manuella et al., 2019; Morrissey & Morrill, 2017; Oskierski, Bailey, et al., 2013; Oskierski et al., 2013a, 2013b; Picazo et al., 2020; Quesnel et al., 2013, 2016; Sánchez‐Murillo et al., 2014; Schwarzenbach et al., 2013, 2016; Ulrich et al., 2014), and on Mars (e.g., Edwards & Ehlmann, 2015; Ehlmann & Edwards, 2014; Ehlmann et al., 2008; Kelemen, Evans, et al., 2020; Salvatore et al., 2018; Tarnas et al., 2021; Tomkinson et al., 2013). References listed here are in addition to studies of carbon mineralization—forming completely carbonated “listvenites”—at the base of the Samail ophiolite mantle section and elsewhere on Earth, summarized in a companion paper to this one (Kelemen, de Obeso, Leong, & Godard, 2021) on OmanDP Hole BT1B, which sampled Cretaceous listvenites at the “leading edge of the mantle wedge,” which formed just above the basal thrus...…”