“…The formations of all three supercontinents reduced the global chemical weathering sink for atmospheric by concentrating the majority of topography production and erosion within the very dry interiors of these landmasses, at large distances from moisture sources (Cox et al, ; Donnadieu et al, ; Fiorella & Poulsen, ; Goddéris et al, ; Otto‐Bliesner, ; Veevers & Powell, ). During the breakups of Pangea and Rodinia, plate reconstructions and geological data suggest that disaggregating supercontinental fragments overran neighboring island arcs forming an initial perimeter (Lee et al, ; Macdonald et al, ; Merdith et al, ; Spencer et al, ). A resulting relatively rapid tectonic transition into continental arc modes is also correlated with large increases in mid‐ocean ridge and arc magmatism (Brandl et al, ; Kelemen & Holbrook, ; Van Avendonk et al, ) and continental arc magmatism (Lee et al, ; McKenzie et al, ) and also marked by extensive orogenesis and chemical weathering occurring close to oceans (e.g., Donnadieu et al, ; Goddéris et al, ; Hartmann et al, ).…”