The Maastrichtian was introduced into scientific literature byBelgian geologistAndré Hubert Dumont in 1849, after studyingrock strata of theChalk Group close to theDutch city ofMaastricht. These strata are now classified as theMaastricht Formation – both theformation and stage derive their names from the city.[6] The Maastricht Formation is known for its fossils from this age, most notably those of the giantsea reptileMosasaurus, which in turn derives its name from the nearby riverMaas (mosa being Latin for the river Maas).[7][8]
The base of the Maastrichtian Stage is at the first appearance ofammonite speciesPachydiscus neubergicus. At the original type locality near Maastricht, the stratigraphic record was later found to be incomplete. A reference profile for the base was then appointed in a section along theArdour river calledGrande Carrière, close to the village ofTercis-les-Bains in southwesternFrance.[2][9] The top of the Maastrichtian Stage is defined to be at theiridium anomaly at theCretaceous–Paleogene boundary (K–Pg boundary), which is also characterised by theextinction of many groups of life.[10]
The breakup ofPangaea was nearly complete in the Maastrichtian, with Australia beginning to break away from Antarctica and Madagascar breaking away from India. However, Arabia had not yet rifted away from Africa. North America was separated from Europe by rift basins, but sea floor spreading had not yet commenced between the two continents.[12]
The Pacific Plate was rapidly growing in size as the surrounding oceanic plates were consumed bysubduction, and the Pacific-Izanagi Ridge was rapidly approaching Asia.[13]
During the Maastrichtian, the global climate began to shift from the warm and humid climate of the Mesozoic to the colder and more arid climate of the Cenozoic.[14] Variation of climate with latitude also became greater. This was likely caused by a major reorganization of oceanic circulation that took place at the boundary between the early and late Maastrichtian. This reorganization was triggered by the breach of tectonic barriers in the South Atlantic, permitting deep ocean water to begin circulating from the nascent North Atlantic to the south. This initiatedthermohaline circulation similar to that of the modern oceans. At the same time, theLaramide orogeny drained theWestern Interior Seaway of North America, further contributing to global cooling.[15] Nonetheless, the latest Maastrichtian featured a sharp, pronounced warming,[16][17] which was caused by the activity of the Deccan Traps.[18]
South-central Alaska had a mean annual temperature of 7.42 ± 1.2 °C, a warm monthly mean temperature of 17.08 ± 1.6 °C, and a cold monthly mean temperature of − 2.31 ± 1.9 °C.[19][20]
Dinosaurs remained the dominant large terrestrial animals throughout the Maastrichtian, though mammals with internal organs similar to modern mammals were also present. Bothammonites andpterosaurs were in serious decline during the Maastrichtian.[21]
Several archaic clades of birds, such asEnantiornithes,Ichthyornithes, andHesperornithes, persisted to the latest Maastrichtian but became extinct during the Cretaceous-Paleogene extinction event.[22]
Traditionally, pterosaur faunas of the Maastrichtian were assumed to be dominated byazhdarchids, with other pterosaur groups having become extinct earlier on. However, more recent findings suggest a fairly composite pterosaur diversity: at least six ("Nyctosaurus"lamegoi, a Mexican humerus, a Jordan humerus and several taxa from Morocco)nyctosaurs date to this period, as do a fewpteranodontids, andNavajodactylus, tentatively assigned to Azhdarchidae, lacks any synapomorphies of the group.[23][24] This seems to underscore a higher diversity of terminal Cretaceous pterosaurs than previously thought.[25][26][27]
The radiation ofangiosperms (flowering plants) was well under way in the Maastrichtian. From 50% to 80% of allgenera of land plants were angiosperms, thoughgymnosperms andferns still covered larger areas of the land surface.[28]
^Torsvik, Trond H.; Cocks, L. Robin M. (2017).Earth history and palaeogeography. Cambridge, United Kingdom: Cambridge University Press. pp. 220, 222, 230.ISBN978-1-107-10532-4.