The Carboniferous is a major division of the geologic timescale that
extends from the end of the Devonian period, about 359.2 ± 2.5 Ma (million years ago), to the beginning of the Permian period, about 299.0 ± 0.8
Ma (ICS 2004). As with most older geologic periods, the rock beds that define the period's start and end are well identified, but the exact dates
are uncertain by 5–10 million years. The Carboniferous is named for the extensive coal beds of that
age found in Western Europe. The first third of the Carboniferous is called the Mississippian epoch, and the remainder is called the
Pennsylvanian. Conifer trees appeared in this important
and well-known time period.
Subdivisions
The Carboniferous is usually broken into Pennsylvanian (later) and Mississippian (earlier) Epochs. The Faunal stages from youngest to oldest, together with some of their subdivisions, are:
Late Pennsylvanian Gzhelian (most recent)
Late Pennsylvanian Kasimovian
- Klazminskian
- Dorogomilovksian/Virgilian
- Chamovnicheskian/Cantabrian/Missourian
- Krevyakinskian/Cantabrian/Missourian
Middle Pennsylvanian Moscovian
- Myachkovskian/Bolsovian/Desmoinesian
- Podolskian/Desmoinesian
- Kashirskian/Atokan
- Vereiskian/Bolsovian/Atokan
Early Pennsylvanian Bashkirian/Morrowan
- Melekesskian/Duckmantian
- Cheremshanskian/Langsettian
- Yeadonian
- Marsdenian
- Kinderscoutian
Late Mississippian Serpukhovian
- Alportian
- Chokierian/Chesterian/Elvirian
- Arnsbergian/Elvirian
- Pendleian
Middle Mississippian Visean
- Brigantian/St Genevieve/Gasperian/Chesterian
- Asbian/Meramecian
- Holkerian/Salem
- Arundian/Warsaw/Meramecian
- Chadian/Keokuk/Osagean/Osage
Early Mississippian Tournaisian (oldest)
- Ivorian/Osagean/Osage
- Hastarian/Kinderhookian/Chautauquan/Chouteau
Paleogeography
A global drop in sea level at the end of the Devonian reversed early in the Carboniferous;
this created the widespread epicontinental seas and carbonate deposition of the
Mississippian.[1] There was also a drop in south polar
temperatures; southern Gondwanaland was glaciated throughout
the period, though it is uncertain if the ice sheets were a holdover from the Devonian or not.[2] These conditions apparently had little effect in the deep tropics, where lush
coal swamps flourished within 30 degrees of the northernmost glaciers.[3]
A mid-Carboniferous drop in sea-level precipitated a major marine extinction, one that hit crinoids and ammonites especially hard.[4] This sea-level drop and the associated unconformity in North America separate the Mississippian period from the Pennsylvanian period.[5]
The Carboniferous was a time of active mountain-building, as the supercontinent Pangaea came together. The southern continents remained tied together in the supercontinent Gondwana, which collided with North America-Europe
(Laurussia) along the present line of eastern North America. This continental collision
resulted in the Hercynian orogeny in Europe, and the Alleghenian orogeny in North America; it also extended the newly-uplifted Appalachians southwestward as the Ouachita
Mountains.[6] In the same time frame, much of
present eastern Eurasian plate welded itself to Europe along the line of the
Ural mountains. Most of the Mesozoic supercontinent of
Pangea was now assembled, although North China (which would collide in the Latest Carboniferous), and South China continents were still separated from Laurasia. The
Late Carboniferous Pangaea was shaped like an "O".
There were two major oceans in the Carboniferous—Panthalassa and Paleo-Tethys, which was inside the "O" in the Carboniferous Pangaea. Other minor oceans were
shrinking and eventually closed - Rheic Ocean (closed by the assembly of South and North America), the small, shallow Ural Ocean (which was closed by the collision of Baltica and Siberia
continents, creating the Ural Mountains) and Proto-Tethys Ocean (closed by North China collision with
Siberia/Kazakhstania.
Climate
The early part of the Carboniferous was mostly warm; in the later part of the Carboniferous, the climate cooled. Glaciations in Gondwana, triggered by Gondwana's southward movement, continued into the Permian and because of the lack of clear markers and breaks, the deposits of this glacial period are often
referred to as Permo-Carboniferous in age.
Rocks and coal
Carboniferous rocks in Europe and eastern North America largely consist of a repeated sequence of limestone, sandstone, shale and
coal beds, known as "cyclothems" in the U.S. and "coal
measures" in Britain.[7] In North America, the early
Carboniferous is largely marine limestone, which accounts for the division of the Carboniferous into two periods in North
American schemes. The Carboniferous coal beds provided much of the fuel for power generation during the Industrial Revolution and are still of great economic importance.
The large coal deposits of the Carboniferous primarily owe their existence to two factors. The first of these is the
appearance of bark-bearing trees (and in particular the evolution of the bark fiber lignin). The second is the lower sea levels that
occurred during the Carboniferous as compared to the Devonian period. This allowed for the
development of extensive lowland swamps and forests in North
America and Europe. Some hypothesize that large quantities of wood were buried during this period
because animals and decomposing bacteria had not yet evolved
that could effectively digest the new lignin. The extensive burial of biologically-produced carbon led to a buildup of surplus oxygen in the atmosphere; estimates place the
peak oxygen content as high as 35%, compared to 21% today.[1] This oxygen level probably increased wildfire
activity, as well as resulted in insect and amphibian
gigantism--creatures whose size is constrained by respiratory systems that are
limited in their ability to diffuse oxygen.
In eastern North America, marine beds are more common in the older part of the period than the later part and are almost
entirely absent by the late Carboniferous. More diverse geology existed elsewhere, of course. Marine life is especially rich in
crinoids and other echinoderms. Brachiopods were abundant. Trilobites became quite uncommon. On land,
large and diverse plant populations existed. Land vertebrates
included large amphibians.
Life
Marine Invertebrates
In the oceans the most important groups are the foraminifera, corals, bryozoa, brachiopods,
ammonoids, echinoderms (especially crinoids), and Chondrichthyes (sharks and their relatives).
For the first time foraminifera take a prominent part in the marine faunas. The large spindle-shaped genus Fusulina and its relatives were abundant in what is now Russia, China, Japan, North America; other
important genera include Valvulina, Endothyra,
Archaediscus, and Saccammina (the latter common in
Britain and Belgium). Some Carboniferous genera are still extant.
The microscopic shells of Radiolaria are found in cherts
of this age in the Culm of Devonshire and Cornwall, and in Russia, Germany and elsewhere.
Sponges are known from spicules and anchor ropes, and include
various forms such as the Calcispongea Cotyliscus and
Girtycoelia, and the unusual colonial glass sponge
Titusvillia.
Both reef-building and solitary corals diversify and flourish; these include both
rugose (e.g. Canina, Corwenia, Neozaphrentis), heterocorals, and tabulate (e.g. Chaetetes, Chladochonus, Michelinia) forms.
Conularids were well represented by Conularia
Bryozoa are abundant in some regions; the Fenestellids
including Fenestella, Polypora, and the remarkable
Archimedes, so named because it is in the shape of an Archimedean screw.
Brachiopods are also abundant; they include Productids,
some of which (e.g. Gigantoproductus) reached very large (for brachiopods) size and had
very thick shells, while others like Chonetes were more conservative in form. Athyridids, Spiriferids, Rhynchonellids, are Terebratulids are also very common.
Inarticulate forms include Discina and Crania. Some
species and genera had a very wide distribution with only minor variations.
Annelids such as Spirorbis and Serpulites are common fossils in some horizons.
Among the mollusca, the bivalves continue to increase in numbers and importance. Typical
genera include Aviculopecten, Posidonomya,
Nucula, Carbonicola, Edmondia, and Modiola
Conocardium is a common rostroconch.
Gastropods are also numerous, including the genera Murchisonia, Euomphalus, Naticopsis.
Nautiloid cephalopods are represented by tightly coiled
nautilids, with straight-shelled and curved-shelled forms becoming increasingly rare.
Goniatite Ammonoids are common.
Trilobites are rare, represented only by the proetid group. Ostracods such as Cythere, Kirkbya, and Beyrichia are abundant.
Amongst the echinoderms, the crinoids were the most
numerous. Dense submarine thickets of long-stemmed crinoids appear to have flourished in shallow seas, and their remains were
consolidated into thick beds of rock. Prominent genera include Cyathocrinus,
Woodocrinus, and Actinocrinus. Echinoids such as
Archaeocidaris and Palaeechinus were also present.
The Blastoids, which included the Pentreinitidae and
Codasteridae and superficially resembled crinoids in the possession of long stalks attached to
the sea-bed, attain their maximum development at this time.
Fish
Many fish inhabited the Carboniferous seas; predominantly Elasmobranchs (sharks and
their relatives). These included some, like Psammodus, with crushing pavement-like teeth
adapted for grinding the shells of brachiopods, crustaceans, and other marine organisms. Other sharks had piercing teeth, such as
the Symmoriida; some, the petalodonts, had peculiar cycloid
cutting teeth. Most of the sharks were marine, but the Xenacanthida invaded fresh waters of
the coal swamps. Among the bony fish, the Palaeonisciformes found in coastal waters also appear to have migrated to rivers. Sarcopterygian fish were also prominent, and one group, the Rhizodonts,
reached very large size.
Most species of Carboniferous marine fish have been described largely from teeth, fin spines and dermal ossicles, with smaller
freshwater fish preserved whole.
Freshwater fishes were abundant, and include the genera Ctenodus, Uronemus, Acanthodes, Cheirodus, and Gyracanthus.
Plants
Early Carboniferous land plants were very similar to those of the preceding Late
Devonian, but new groups also appeared at this time.
The main Early Carboniferous plants were the Equisetales (Horse-tails), Sphenophyllales (vine-like plants), Lycopodiales (Club mosses),
Lepidodendrales (scale trees), Filicales (Ferns), Medullosales (informally included in the "seed ferns", an
artificial assemblage of a number of early gymnosperm groups) and the Cordaitales. These continued to dominate throughout the period, but during late Carboniferous, several other groups, Cycadophyta (cycads), the
Callistophytales (another group of "seed ferns"), and the Voltziales (related to and sometimes included under the conifers),
appeared.
The Carboniferous lycophytes of the order Lepidodendrales, which are cousins (but not ancestors) of the tiny club-moss of
today, were huge trees with trunks 30 meters high and up to 1.5 meters in diameter. These included Lepidodendron (with its fruit cone called Lepidostrobus),
Halonia, Lepidophloios and Sigillaria. The roots of several of these forms are known as Stigmaria.
The fronds of some Carboniferous ferns are almost identical with those of living species. Probably many species were
epiphytic. Fossil ferns and "seed ferns" include Pecopteris, Cyclopteris, Neuropteris, Alethopteris, and Sphenopteris; Megaphyton and Caulopteris were tree ferns.
The Equisetales included the common giant form Calamites, with a trunk diameter of
30 to 60 cm and a height of up to 20 meters. Sphenophyllum was a slender climbing plant
with whorls of leaves, which was probably related both to the calamites and the lycopods.
Cordaites, a tall plant (6 to over 30 meters) with strap-like leaves, was related to
the cycads and conifers; the catkin-like inflorescence, which bore yew-like berries, is called
Cardiocarpus. These plants were thought to live in swamps and mangroves. True coniferous
trees (Waichia, of the order Voltziales) appear later in the Carboniferous, and preferred
higher drier ground.
Freshwater and Lagoonal Invertebrates
Freshwater Carboniferous invertebrates include various bivalve molluscs that lived in brackish or fresh water, such as Anthracomya,
Naiadiles, and Carbonicola; diverse
crustaceans such as Bairdia, Carbonia, Estheria, Acanthocaris, Dithyrocaris, and Anthrapalaemon.
The Eurypterids were also diverse, and are represented by such genera as
Eurypterus, Glyptoscorpius, Anthraconectes, Megarachne (originally misinterpreted as a
giant spider) and the specialised very large Hibbertopterus. Many of these were
amphibious.
Frequently a temporary return of marine conditions resulted in marine or brackish water genera such as Lingula, Orbiculoidea, and Productus
being found in the thin beds known as marine bands.
Terrestrial Invertebrates
Fossil remains of air-breathing insects, myriapods and
arachnids are known from the late Carboniferous, but so far not from the early Carboniferous.
Their diversity when they do appear however show that these arthropods were both well developed and numerous. Their large size
can be attributed to the moistness of the environment (mostly swampy fern forests) and the fact that there was a 36% higher
oxygen concentration in Earth's atmosphere than today, requiring less effort for respiration and allowing arthropods to grow larger. Among the insect groups are the Syntonopterodea
(relatives of present-day mayflies), the abundant and often large sap-sucking Palaeodictyopteroidea, the huge predatory Protodonata
(griffinflies), the diverse herbivorous "Protorthoptera", and numerous basal Dictyoptera (ancestors of cockroaches). Many insects have been obtained from the coalfields of Saarbruck
and Commentry, and from the hollow trunks of fossil trees in Nova Scotia. Some British
coalfields have yielded good specimens: Archaeoptitus, from the Derbyshire coalfield, had
a spread of wing extending to more than 35 cm; some specimens (Brodia) still exhibit
traces of brilliant wing colors. In the Nova Scotian tree trunks land snails (Archaeozonites, Dendropupa) have been found.
Tetrapods
Carboniferous amphibians were diverse and common by the middle of the period, more so than
they are today; some were as long as 6 meters, and those fully terrestrial as adults had scaly skin.[8] They included a number of basal tetrapod groups classified in early books under
the Labyrinthodontia. These had long bodies, a head covered with bony plates and
generally weak or undeveloped limbs. The largest were over 2 meters long. They were accompanied by an assemblage of smaller
amphibians included under the Lepospondyli, often only about 15 cm long. Some Carboniferous
amphibians were aquatic and lived in rivers (Loxomma, Eogyrinus, Proterogyrinus); others may have been
semi-aquatic (Ophiderpeton, Amphibamus) or
terrestrial (Dendrerpeton, Hyloplesion,
Tuditanus, Anthracosaurus).
Pederpes finneyae, the most primitive Mississippian tetrapod
One of the greatest evolutionary innovations of the Carboniferous was the amniote egg, which
allowed for the further exploitation of the land by certain tetrapods. These
included the earliest Sauropsid reptiles (Hylonomus), and the earliest known synapsid (Archaeothyris). These small lizard-like animals quickly gave rise to many descendants. The amniote egg
allowed these ancestors of all later birds, mammals, and
reptiles to reproduce on land by preventing the desiccation, or drying-out, of the
embryo inside. By the end of the Carboniferous period, the amniotes had already diversified into a number of groups, including protorothyridids, captorhinids, aeroscelids, and several families of pelycosaurs.
Fungal life
Because plants and animals were growing in size and abundance in this time (e.g., Lepidodendron), land fungi diversified further. Marine fungi still
occupied the oceans.
Extinction events
The Middle Carboniferous extinction event is shown here as
Middle C.
In the middle Carboniferous, an extinction event occurred that was probably caused
by climate change. A less intense extinction event also occurred by the end of
Carboniferous.
See also
Footnotes
- ^ Steven M. Stanley, Earth System History. (New York: W.H. Freeman and
Company, 1999), 414.
- ^ Stanley, 414.
- ^ Stanley, 416.
- ^ Stanley, 414.
- ^ Stanley, 414.
- ^ Stanley, 414-6.
- ^ Stanley, 426.
- ^ Stanley, 411-12.
References
- Stanley, Steven M. Earth System History. New York: W.H. Freeman and Company, 1999. ISBN 0-7167-2882-6
This article incorporates text from the Encyclopædia
Britannica Eleventh Edition, a publication now in the public
domain.
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