“…Meteoric diagenesis is also important to the evolution of matrix-scale poresystems in rocks that have undergone dolomitization. Examples include 'dedolomitization' or the replacement of dolomite by calcite (Frank, 1981;Kupecz et al, 1993;Nader et al, 2008;Rameil, 2008;Vandeginste & John, 2012) commonly in the presence of calcium sulphate dissolution (Von Morlot, 1847;Bischoff et al, 1994;Arenas et al, 1999;Hauck et al, 2018) and the formation of hollow dolomite rhombs (Jones et al, 1989;Youssef, 1997;Ryan et al, 2019). Dolomite dissolution in the meteoric realm has also been implicated in the formation of dolomitic sediment variably referred to as 'pulverulent chalk' (Blank & Tynes, 1965), 'pulverulite' (Rose, 1972;Chafetz & Butler, 1980;Kahle, 2012), 'crushed dolomite' (Zogovi c, 1966), 'flour dolomite' (Ji et al, 2004), 'dolomite powder' (Machel et al, 2012), 'dolomite silt' (Hajna, 2003), 'dolomite sand' (James et al, 1993;Richter et al, 2018) and 'disintegrated dolomite' (Richter et al, 2018).…”