Carbonates are common rock-forming minerals in the Earth's crust and act as sinks of atmospheric carbon dioxide (CO 2 ) released from the mantle through volcanism. Subduction of hydrothermally altered oceanic lithosphere returns carbonates and organic matter from near-surface reservoirs to the interior, where more than three quarters of Earth's carbon is stored (e.g. Chen et al., 2014;Dasgupta & Hirschmann, 2010). A significant fraction of the subducted carbonates will join shallow cycles within the top 200 km of the solid Earth, whereas the rest reaches greater depths to participate in deep cycles, possibly extending to the core (Dasgupta & Hirschmann, 2010;Kelemen & Manning, 2015). The long-term evolution of CO 2 in the atmosphere is influenced by the residence time of carbonates in solid Earth, which, in turn, depends on their melting behavior and chemical stability under relevant conditions.Calcium carbonate (CaCO 3 ), dolomite (CaMg[CO 3 ] 2 ), and magnesium carbonate (MgCO 3 ) are dominant ingredients in subducted slabs (e.g. Alt & Teagle, 1999). Although magnesite is expected to be the ultimately stable carbonate in the deep mantle (Biellmann et al., 1993;Keshav et al., 2011;Kushiro et al., 1975;Yaxley & Brey, 2004), Ca-carbonate in fast-descending slabs may be preserved to reach the mantle transition zone (MTZ) or lower mantle, as indicated by calcite and nyerereite (Na-K-Ca bicarbonate) inclusions in superdeep diamonds from Juina, Brazil (Brenker et al., 2007;Kaminsky et al., 2009). The MTZ is widely considered a potential water reservoir and known to be at least locally wet, as indicated by hydrous ringwoodite and ice VII inclusions in superdeep diamonds (