The Cretaceous world: plate tectonics, palaeogeography and palaeoclimate

Abstract

The tectonics, geography, and climate of the Cretaceous world was a very different from the modern world. At the start of the Cretaceous, the supercontinent of Pangea had just begun to break apart and only a few small ocean basins separated Laurasia, West Gondwana, and East Gondwana. Unlike the modern world, there were no significant continent-continent collisions during the Cretaceous and the continents were low-lying and easily flooded. The transition from a Pangea-like configuration to a more dispersed continental arrangement had important effects on global sea level and climate. During the Early Cretaceous, as the continents rifted apart, the new continental rifts were transformed into young ocean basins. The oceanic lithosphere in these young ocean basins was thermally elevated, which boosted sea level. Sea level, on average, was ∼70 m higher than the present-day. Sea level was highest during the mid-Cretaceous (90 Ma – 80 Ma), with a subsidiary peak ∼ 120 million years ago (early Aptian). Overall, the Cretaceous was much warmer than the present-day (> 10˚C warmer). These very warm times produced oceanic anoxic events (OAEs) and high temperatures in equatorial regions sometimes made terrestrial and shallow marine ecosystems uninhabitable (temperatures > 40˚C). This is unlike anything we have seen in the last 35 million years and may presage the eventual results of man-made global warming. This mostly stable, hot climate regime endured for nearly 80 million years before dramatically terminating with the Chicxulub bolide impact 66 million years ago. Temperatures plummeted to icehouse levels in the “impact winter” resulting from sunlight-absorbing dust and aerosols. As a consequence of the collapse of the food chain, ∼75% of all species were wiped out (Sepkoski, 1996). The effect of this extinction event on global ecosystems was second only to the great Permo-Triassic Extinction (McGhee et al., 2013).