“…Earth's impact craters larger than *2 to 4 km in diameter are of complex morphology and structure, such as the *3.8 km-diameter Steinheim Basin in Germany characterized by a pronounced central peak (uplift) and the *25 km-diameter Nördlinger Ries with an *10 km-wide inner ring of uplifted target rock and a well-preserved blanket of proximal impact ejecta surrounding the crater (e.g., Stöffler et al, 2002Stöffler et al, , 2013Kring, 2005;. The 180 km-diameter Chicxulub crater on the Yucatán Peninsula in Mexico is a peak-ring basin similar in morphology and structure to the Schrödinger Basin on the Moon (Kring, 1995;Kring et al, 2016Kring et al, , 2017aMorgan et al, 2016). The deeply eroded Vredefort impact structure in South Africa, probably *250 to 300 km in original diameter, may represent the remnants of a terrestrial multiring basin (e.g., Melosh, 1989;Spudis, 1993;Therriault et al, 1997;French, 1998).…”