Stable carbon isotope data from Late Cretaceous (Maastrichtian) palaeo
sols in India are used to estimate the concentration of carbon dioxide
in the Late Cretaceous atmosphere. We show that the Maastrichtian atm
osphere is unlikely to have contained more than about 1300 ppm by volu
me of CO2, This value agrees with an independently modelled value of C
O2 in the Late Cretaceous atmosphere. A low concentration of the green
house gas carbon dioxide in the Maastrichtian atmosphere (relative to
concentrations in the earlier Cretaceous) is consistent with palaeotem
perature information from terrestrial plant and marine fossils, which
suggest that the global climate cooled toward the end of the Cretaceou
s Period.