“…Given the general supposition, using oxygen-isotope paleothermometry and faunal/ floral distributions, that the Maastrichtian was globally cooler than the preceding mid and Late Cretaceous stages (for example, Voigt, 1964;Naydin, Teys, and Zadorozhnyy, 1966;Douglas and Savin, 1975;Wolfe and Upchurch, 1987;Kolodny and Raab, 1988;Arthur, Dean, and Schlanger, 1985;Spicer and Parrish, 1990;Clauser, 1994;Ditchfield, Marshall, and Pirrie, 1994;Huber, Hodell, and Hamilton, 1995), it seems likely that equatorial sea-surface temperatures were above 30°C during the Albian-Campanian interval. This view is consistent with paleotemperature determinations from planktonic foraminifera from the Cretaceous of the Pacific (Price and others, 1998) and Atlantic (Norris and Wilson, 1998) as well as with extrapolated southern-hemisphere paleotemperature trends (Clarke and Jenkyns, 1999).…”