Palaeos: Mesozoic Palaeos Late Cretaceous I
Cretaceous Period

The Santonian Age

The Santonian Age of the Late Cretaceous Period: 85.8 to 83.5 million years ago


Geography of the Santonian

Africa & Eurasia in the SantonianThe geography of the Santonian seems to be a contentious subject.  One version of the African and Mediterranean region is shown here.  This map shows the position of the tectonic plates, with modern shorelines superimposed for reference.  However, the Santonian was a time of extremely high sea levels -- perhaps the highest ever -- and much of the area shown as "land" would have been covered by shallow seas.  You may get an idea of the proportions by looking at the PaleoMap Project map of the Late Cretaceous (Cenomanian).  Dr. Blakey's maps of the Late Cretaceous are perhaps the best overall representation.  

On the whole, the globe was beginning to look quite familiar by the Santonian, with a few exceptions.  The Atlantic was narrower than in modern times.  In fact, there may be some dispute as to whether the South Atlantic was entirely open yet.  Some residual contact between the continental shelves of South America and Africa may have remained.  However, the Central Atlantic was certainly open.  The situation north of the Central Atlantic is less certain.  Probably, an open seaway continued right up to the North Pole through the Labrador Sea.  The Atlantic waters were certainly connected with the Pole by way of the North American Interior Seaway, which cut right through the center of the North American continent.  South America, and even perhaps Africa, also held substantial inland seas.  

Although the Atlantic was becoming quite recognizable, Southern Europe was still a confused and poorly understood collection of microplates, most of which were submerged, as were large sections of Eurasia.  The Tethys Seaway through this region remained well open, and a strong westerly current swept from the Tethys, out across the Labrador Sea to South America.  The Arabian peninsula remained tightly bound to Africa.  India, which would one day close the Eastern end of the Tethys, was still far away.  At this point in time, India was just separating from Madagascar and beginning its sprint (by geological standards) toward South Asia.  

Eastern Asia had, by this time, consolidated, although Japan was probably still well to the South of its present position, perhaps just north of the equator.  Australia was firmly locked to Antarctica, which was a bit east of its present position.  The Pacific was far larger even than its present size, since most major land masses were still fairly well bunched near their Pangean positions. 

Across the Pacific, the Sevier orogeny was beginning to build the Rocky Mountains in earnest, just as the Andes were becoming a major mountain chain in South America.  The present Central America was open ocean.  However, North and South America may have been sporadically joined through the Caribbean Arch.  

Image: from Geodynamic evolution of the Alpine Tethys.  ATW030206.

Climate of the Santonian

The Santonian may have been an age of storms.  This speculation is admittedly our own, but there are several, independent lines of evidence that point to this conclusion.  

First, several conditions were extremely favorable to the formation of cyclonic storms.  World temperatures were both hot and uniform.  There is considerable disagreement about the pattern of temperature change in the Late Cretaceous, but there is no doubt that it was very warm by modern standards.  The Santonian is particularly noted for its even temperatures.  That is, the average temperature varied little from pole to pole.  It is not clear why this should be so, but the evidence from isotope ratios and the distribution of planktonic microfossils (and dinosaurs, for that matter!) is very clear.  We may add to this mixture the highest sea levels the world had ever experienced, at least during Phanerozoic times.  The net result is millions of square kilometers of open ocean, much of it shallow and easily warmed, baking to temperatures over 26.5 C., the critical water temperature for hurricane formation.  Because temperatures were hot, humid, and uniform, we would be unlikely to see temperature inversions or complex upper air flows (causing vertical wind shear), both of which tear hurricanes apart before they can form.  

Second, the Santonian was notable for the controversial phenomenon of black shales.  Black shales are dark layers of poorly oxidized decomposed organic matter on the ocean floor.  There has been much discussion of the reasons for supposed Ocean Anoxic Events (OAEs) which caused these materials to accumulate.  The supposition generally is that hot, uniform ocean surface temperatures created very stable layering of the oceans, depleting the oxygen in cooler deep ocean waters.  However, OAEs seem to be made up of very short intervals of anoxic accumulation.  We will not get far into this highly technical debate. The point we wish to make is that one possible reason for the perceived pattern of OAEs is that organic matter accumulated in large bursts and was buried  quickly, before it could decompose.  This might occur where giant storms washed enormous amounts of continental plant material into the ocean within days.  This hypothesis accounts for both the presence and pattern of black shales.  It also accounts for external link recent findings in Venezuela which show long periods of black shale accumulation outside the established Atlantic OAEs.  Venezuela is roughly where one might expect ordinary tropical storms to make landfall in the Santonian.  The presence of black shales in this region, outside the known temporal range of OAEs is consistent with hurricane events as the root cause of black shale accumulation.

Third, we know of another direct measure of storm activity, this time from North America.   Dr. James Lamb of North Carolina State University has external link sampled Santonian vegetation in the Southeastern United States and along the north coast of the Gulf of Mexico. He finds that the northern Gulf differs from most contemporary sites because the tree-sized vegetation is dominated by pines.  He believes that this is due to the influence of storm activity which periodically cleaned out the entire crop of standing trees, allowing the faster-growing pines to maintain an unstable dominance over angiosperm trees in this region.   If correct, this provides relatively direct evidence of very large storm activity on a reasonably regular basis.

Much of the recent literature has been devoted to examining the relationship between OAEs and long cycles in Earth's orbit around the sun.  This may well be the case, as these cycles have large, if poorly understood, effects on Earth's weather.  But whatever the root geophysical cause, we suggest that the immediate cause was sudden accumulation of vast amounts of organic debris through hurricane activity.  The climatic conditions and physical evidence point to the Santonian as an age of violent storms.  ATW030205.

Representative Ecological Communities

The following reconstruction of a Santonian Micraster Chalk Community is from W. S. McKerrow The Ecology of Fossils


Santonian Micraster Chalk Community
a Parapuzosia (Mollusca - Cephalopoda - Ammonoidea)
b Ventriculites (Porifera - Hyalospongea)
c Echinocorys scutata (Echinodermata - Echinoidea)
d Micraster (Echinodermata - Echinoidea)
e Conulus albogalerus (Echinodermata - Echinoidea)
f Baurgueticrinus eltipticus (Echinodermata - Crinoidea)
g Mitraster hunteri (Echinodermata - Asteroidea)
h Spondylus spinosus (Mollusca - Bivalvia - Pterioida)
i Inoceramus fragments (Mollusca - Bivalvia - Pterioida
j Pycnodonte vesicutaris (Mollusca - Bivalvia - Pterioida - Oyster)
k Parasmilia centralis (Cnidaria - Anthozoa: Scleractinia)
I serpulids (Annelida)
m bryozoans (Bryozoa)
n Gibbithyris (Brachipoda - Articulata: Terebratulida)
o Cretirhynchia (Brachipoda - Articulata: Rhynchonellida)
p Ptychodus tooth (Vertebrata - Chondrichthyes)
q Tylocidaris clavigera (Echinodermata - Echinoidea)

"The reconstruction of this fauna assemblage is based on a highly fossiliferous soft Santonian chalk on the Kent coast. Faunas of this general composition occur throughout much of the English Upper Chalk, but elsewhere faunal densities are very much lower.

The chalk has been intensively bioturbated, but is so pure that burrow outlines are difficult to detect. Bottoms were probably thixotropic or semi-fluid, and the faunal elements present show adaptations to this habitat. All but the largest aragonitic organisms are absent.

Benthic elements frequently adapted themselves for living on soft bottoms: they sometimes developed long spines to spread the weight of the shell, as in the case of the pectinid Spondylus [h], or club-shaped spines, as with the cidarid echinoid Tylocidaris [q]. Inoceramids are scarce; when present they have often developed a bowl-like lower valve, or are vastly expanded and flattened. Shell debris provided hard substrates which were heavily encrusted by bryozoans [m], serpulids and oysters; they may also have provided a substrate for some brachiopods. Other brachiopods such as Cretirhynchia [o], lay loose on the sediment surface when adult. Echinoderms are a prominent element of these faunas and shown here are Micraster [d], an infaunal or semi-infaunal deposit feeder; Conulus [c] and Echinocorys [c], which probably lived partly buried, ploughing through sediment and feeding on detritus; the cushion star Mitraster [g] and the crinoid Bourgueticrinus [f]. Nekton are represented by the giant ammonite Parapuzasia [a] which reaches a diameter close to 2 metres, and by teeth of the mollusk-eating fish Ptychodus [p] (tooth), probably responsible for much of the fragmentation of inoceramids and other shells."

© xxxx - W.J. Kennedy "Cretaceous", in W.S. McKerrow (ed.) The Ecology of Fossils pp. 318-9

The Mosasaur Success Story Continues

Tylosaurus skull Although these huge marine lizards had only first appeared a few million years earlier, they had already by Santonian times attained a great ecological diversity. The three subfamilies continue and each are well represented in the Niobrara Chalk.

Clidastes propython is a primitive member of the subfamily Mosasaurinae [DeBraga and Carroll 1993 p.252]. It was the smallest mosasaur of the North American inland sea, with an average length of about 4 meters, and a slender elongated body and a relatively short flattened tail. The end of tail features expanded neural spines that created a tail-fin, although the existence of an additional soft-tissue fin (as possessed by sea-snakes) to further enlarge the end of tail is debatable. In any case Clidastes was a fast swimmer, and possibly able to dive to fairly great depths [Creisler 2000]

Tylosaurus propriger is a very large mosasaur, with lengths of up to 10 to 12 meters and a skull alone of upto a meter or more. (Tylosaurus skull illustrated above). Clearly this was the dominant animal in its environment. It is representative of the second subfamily, Tylosaurinae. It is named for its long projecting snout, or rostrum, which projects past the front teeth in the upper jaw; and may have been similar in function to the "ram" or "beak" (Lat. rostrum) that the ancient Greeks and Romans mounted on the prow of warships to sink enemy vessels. Tylosaurus might have use its snout to ram and stun prey, defend against sharks or other predators, and battle rivals of its own species. [Creisler 2000]

Platecarpus ictericus - A medium-sized species, 4.3 meters in length, Platecarpus belongs to the most advanced subfamily of mosasaurs, the Plioplatecarpinae. This was a common species in the Inland Sea that became the Niobrara chalk deposits. The flattened tail is as long as the body, and the animal swum with a sinuous motion, while the broad feet were used for steering [Cox et al pp.88-89]. Although the thick fossilized eardrums would seem to indicate a deep-diving capacity [Williston 1898 ], these animals appear to have been adapted to life in shallow water as an ambush predator [Creisler 2000] MAK030211

Technical Notes on Mosasaurs Some Technical Notes on Mosasaurs


Pterosaurs and Birds

Pteranodon ingens

The giant pterosaur Pteranodon ingens, with a wingspan of 7 meters, dwarfs the toothed shore birds (Ichthyornis) with which it shared its environment

from Early Images
(this image is public domain - the copyright has expired)

Throughout the Cretaceous, pterosaurs grew larger, while the ecological niche of smaller fish and insect-eaters that during the Jurassic was occupied by Rhamphorhynchid and other small pterosaurs is now occupied by true birds.


Hadrosaurid Dinosaurs

Claosaurus agilis

drawing © 2000 Vince R Ward - Prehistoric Pages

It can be assumed that Santonian dinosaurs were not very different to those of the preceding Coniacian age, but seem to be poorly represented in the fossil record. Mongolian sediments seem to be either older (Coniacian or at latest Early Santonian) or younger (Middle Campanian onwards), although admittedly the stratigraphy is still uncertain. Brazilian dinosaurs may also tentatively be of Santonian age although again the dating is not certain. The Nequen Formation of Argentina may be either Coniacian or Santonian. So the only certain dinosaurs of this age are a few rare specimens from the Niobrara that were washed out to sea before being fossilized, and even their the dating may be anywhere from Middle Santonian to Early Campanian.

The Laurasian Hadrosauridae, which go back as far as the Cenomanian, were wide-spread but primitive, as indicated by Claosaurus agilis from the Niobrara of Kansas (sketch, above) a small (3.5 meters long) animal known from a mostly complete postcranium and some skull fragments. Claosaurus is one of the most primitive hadrosaurids known, as it retains of the first metatarsal, which all other hadrosaurids for which the foot is known have lost. [Tweet iNet]. It may be compared with Asian species such as Arstanosaurus of the Bayn Shireh Formation (Svita), Gobi Desert, Mongolia (probably Turonian or Coniacian), Gilmoreosaurus mongoliensis and Bactrosaurus johnsoni from the Iren Dabasu Formation of Inner Mongolian (dating uncertain, perhaps anywhere from Turonian to Campanian). Gilmoreosaurus was a large animal (possibly upto 8 meters), with an iguanodont-like skull, that represents the beginning of, or is prior to, the hadrosaurine lineage. Bactrosaurus (4 to 6 meters long) is almost as primitive, and stands at the base of lambeosaurine (hollow-crested duckbills) evolution. The very primitive Telmatosaurus transylvanicus (Nopcsa, 1899), a smallish (5 meters long) animal known from fragmentary skulls and postcrania from Romania, France and Spain, lived much later, during the late Maastrichtian, but had an Iguanodont-like skull and is one of the few known European hadrosaurs. The contemporary Argentine Secernosaurus koerneri, only 3 meters long, may have been at a similar level of organization and is one of only two known Gondwana hadrosaur species

It seems then that during or prior to (perhaps in the Turonian or Coniacian) this time, primitive hadrosaurs migrated widely, colonizing Eastern Laurasia (Europe and Eastern North America), and Gondwana. While the center of Hadrosaurid evolution, like ankylosaurid, ceratopsid, pachycephalosaurid, tyrannosaurid, and maniraptoran evolution, remained the huge Asiamerican island (a long strip of land from Mongolia through to Western Canada and down to Mexico), these other regions, dominated by a saurischian Titanosaurid-Abelisaurid megafauna, proved a welcoming environment for the very primitive Hadrosaurs, which persisted seemingly with little change right up until the end of the age of the Dinosaurs. MAK030211


Links

Web links Links Web links

drawingLate CretaceousDr Ron Blakey's Global Earth History

Web Site Oceans of Kansas - Mike Everhart's world-class site, which includes a great deal of material about the Niobrara (mid Santonian to Early Campanian)

photos Colorado Niobrara Formation fossils - from the Itano website

photos Santonian (Late Cretaceous) Cephalopods - photos of some large ammonites - from Kevin Bylund's Old Calamari - Fossil Cephalopods in Utah website

photos Upper Cretaceous Sharks & Rays of Kansas - Mike Everhart

Chronological List of Taxa -Santonian - from The Plesiosaur Site

DinoData - Santonian - list of dinosaurs from this period (note - because of uncertainty in stratigraphic dating, not all the species listed on the page are necessarily of this time-period

Between the Devil and the Deep Blue Sea - Brandi Berry provides a short description of a number of taxa from the Niobrara


 






page uploaded on Palaeos Site 9 April 2002, last modified 11 February 2003
checked ATW031114
original material copyleft Copyleft Toby White (ATW) and M. Alan Kazlev (MAK) 2003
this material may be freely used
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