Megafauna

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The African bush elephant, Earth's largest living land animal

In terrestrial zoology, megafauna (Ancient Greek megas "large" + New Latin fauna "animal") are "giant", "very large" or "large" animals. The most common thresholds used are 44 kilograms (100 lb)[1][2] or 100 kilograms (220 lb).[2][3] This thus includes many species not popularly thought of as overly large, such as white-tailed deer and red kangaroo, and for the lower figure, even humans.

In practice the most common usage encountered in academic and popular writing describes land animals roughly larger than a human which are not (solely) domesticated. The term is especially associated with the Pleistocene megafauna — the giant and very large land animals considered archetypical of the last ice age such as mammoths.[4] It is also commonly used for the largest extant wild land animals, especially elephants, giraffes, hippopotamuses, rhinoceroses, elk, condors, etc. Megafauna may be subcategorized by their trophic position into megaherbivores (e.g. elk), megacarnivores (e.g. lions), and more rarely, megaomnivores (e.g. bears).

Other common uses are for giant aquatic species, especially whales, any larger wild or domesticated land animals such as larger antelope and cattle, and dinosaurs and other extinct giant reptilians.

The term is also sometimes applied to animals (usually extinct) of great size relative to a more common or surviving type of the animal, for example the 1 m (3 ft) dragonflies of the Carboniferous period.

Contents

[edit] Ecological strategy

Megafauna — in the sense of the largest mammals and birds — are generally K-strategists, with great longevity, slow population growth rates, low death rates, and few or no natural predators capable of killing adults. These characteristics, although not exclusive to such megafauna, make them highly vulnerable to human overexploitation.

[edit] Evolution of large body size

One observation that has been made about the evolution of larger body size is that rapid rates of increase that are often seen over relatively short time intervals are not sustainable over much longer time periods. In an examination of mammal body mass changes over time, the maximum increase possible in a given time interval was found to scale with the interval length raised to the 0.25 power.[5] This is thought to reflect the emergence, during a trend of increasing maximum body size, of a series of anatomical, physiological, environmental, genetic and other constraints that must be overcome by evolutionary innovations before further size increases are possible. A strikingly faster rate of change was found for large decreases in body mass, such as may be associated with the phenomenon of insular dwarfism. When normalized to generation length, the maximum rate of large body mass decreases was found to be over 30 times greater than the maximum rate for large body mass increases.[5]

[edit] In terrestrial mammals

Subsequent to the K-T extinction event that eliminated the dinosaurs about 65.5 Ma ago, terrestrial mammals underwent a nearly exponential increase in body size as they diversified to occupy the ecological niches left vacant.[6] Starting from just a few kg before the event, maximum size had reached ~50 kg a few million years later, and ~750 kg by the end of the Paleocene. This trend of increasing body mass appears to level off about 40 Ma ago (in the late Eocene), suggesting that physiological or ecological constraints had been reached, after an increase in body mass of over three orders of magnitude.[6] However, when considered from the standpoint of rate of size increase per generation, the exponential increase is found to have continued until the appearance of Indricotherium 30 Ma ago. (Since generation time scales with body mass0.259, increasing generation times with increasing size cause the log mass vs. time plot to curve downward from a linear fit.)[5]

Megaherbivores eventually attained a body mass of over 10 000 kg. The largest of these, indricotheres and proboscids, have been hindgut fermenters, which are believed to have an advantage over foregut fermenters in terms of being able to accelerate gastrointestinal transit in order to accommodate very large food intakes.[7] A similar trend emerges when rates of increase of maximum body mass per generation for different mammalian clades are compared (using rates averaged over macroevolutionary time scales). Among terrestrial mammals, the fastest rates of increase occurred in perissodactyls, followed by rodents and proboscids,[5] all of which are hindgut fermenters. The rate of increase for artiodactyls was about a third that of perissodactyls. The rate for carnivorans was slightly lower yet, while primates, perhaps constrained by their arboreal habits, had the lowest rate among the mammalian groups studied.[5]

Terrestrial mammalian carnivores from several eutherian groups (the mesonychid Andrewsarchus, the creodonts Megistotherium and Sarkastodon, and the carnivorans Amphicyon and Arctodus) all reached a maximum size of about 1000 kg[6] (Arctotherium apparently actually got a bit larger). The largest known metatherian carnivore, Proborhyaena gigantea, apparently reached 600 kg, also close to this limit.[8] A similar theoretical maximum size for mammalian carnivores has been predicted based on the metabolic rate of mammals, the energetic cost of obtaining prey, and the maximum estimated rate coefficient of prey intake.[9] It has also been suggested that maximum size for mammalian carnivores is constrained by the stress the humerus can withstand at top running speed.[8]

Analysis of the variation of maximum body size over the last 40 Ma suggests that decreasing temperature and increasing continental land area are associated with increasing maximum body size. The former correlation would be consistent with Bergmann's rule,[10] and might be related to the thermoregulatory advantage of large body mass in cool climates,[6] better ability of larger organisms to cope with seasonality in food supply,[10] or other factors;[10] the latter correlation could be explainable in terms of range and resource limitations.[6] However, the two parameters are interrelated (due to sea level drops accompanying increased glaciation), making the driver of the trends in maximum size more difficult to identify.[6]

[edit] In flightless birds

During the Paleocene, because of the small initial size of all mammals, apex predator niches were often occupied by members of other classes, such as terrestrial crocodilians (e.g. Pristichampsus), large snakes (e.g. Titanoboa), varanid lizards, or flightless birds[6] (e.g. Gastornis in Europe and North America, Paleopsilopterus in South America). In the northern continents, large predatory birds were displaced when large eutherian carnivores evolved. In isolated South America, the phorusrhacids could not be outcompeted by the local metatherian sparassodonts and remained dominant until advanced eutherian predators arrived from North America (as part of the Great American Interchange) during the Pliocene. However, none of the largest predatory (Brontornis), possibly omnivorous (Dromornis[11]) or herbivorous (Aepyornis) flightless birds of the Cenozoic ever grew to masses much above 500 kg, and thus never attained the size of the largest mammalian carnivores, let alone that of the largest mammalian herbivores. It has been suggested that the increasing thickness of avian eggshells in proportion to egg mass with increasing egg size places an upper limit on the size of birds.[12] The largest species of Dromornis, D. stirtoni, may have gone extinct after it attained the maximum avian body mass and was then outcompeted by marsupial diprotodonts that evolved to sizes several times larger.[13]

[edit] Mass extinctions

A well-known mass extinction of megafauna, the Holocene extinction (see also Quaternary extinction event), occurred at the end of the last ice age glacial period (a.k.a. the Würm glaciation) and wiped out many giant ice age animals, such as woolly mammoths, in the Americas and northern Eurasia. Various theories have attributed the wave of extinctions to human hunting, climate change, disease, a putative extraterrestrial impact, or other causes. However, this extinction pulse near the end of the Pleistocene was just one of a series of megafaunal extinction pulses that have occurred during the last 50,000 years over much of the Earth's surface, with Africa and southern Asia being largely spared. (The latter areas did suffer a gradual attrition of megafauna, particularly of the slower-moving species, over the last several million years.[14][15]) Outside the mainland of Afro-Eurasia, these megafaunal extinctions followed a distinctive landmass-by-landmass pattern that closely parallels the spread of humans into previously uninhabited regions of the world, and which shows no correlation with climate.[16][17] Australia was struck first around 46,000 years ago,[18] followed by Tasmania about 41,000 years ago (after formation of a land bridge to Australia about 43,000 years ago),[19][20][21] Japan apparently about 30,000 years ago,[22] North America 13,000 years ago, South America about 500 years later,[23][24] Cyprus 10,000 years ago,[25][26] the Antilles 6000 years ago,[27] New Caledonia[28] and nearby islands[29] 3000 years ago, Madagascar 2000 years ago,[30] New Zealand 700 years ago,[31] the Mascarenes 400 years ago,[32] and the Commander Islands 250 years ago.[33] Nearly all of the world's isolated islands could furnish similar examples of extinctions occurring shortly after the arrival of Homo sapiens, though most of these islands, such as the Hawaiian Islands, never had terrestrial megafauna, so their extinct fauna were smaller.[16][17]

Continuing human hunting and environmental disturbance has led to additional megafaunal extinctions in the recent past, and has created a serious danger of further extinctions in the near future (see examples below).

A number of other mass extinctions occurred earlier in Earth's geologic history, in which some or all of the megafauna of the time also died out. Famously, in the Cretaceous–Tertiary extinction event the dinosaurs and most other giant reptilians were eliminated. However, the earlier mass extinctions were more global and not so selective for megafauna; i.e., many species of other types, including plants, marine invertebrates[34] and plankton, went extinct as well. Thus, the earlier events must have been caused by more generalized types of disturbances to the biosphere.

[edit] Effect of megafaunal extinctions on methane emissions

Many herbivores produce methane as a byproduct of foregut fermentation in digestion, and release it through belching. Large populations of herbivore megafauna have the potential to contribute greatly to the atmospheric concentration of methane, which is an important greenhouse gas. Today, around 20% of annual methane emissions come from livestock methane release. Recent studies have indicated that the extinction of megafaunal herbivores may have caused a reduction in atmospheric methane. This hypothesis is relatively new.[35]

Several studies have examined the effect of elimination of megaherbivorous mammals on methane emissions. One study examined the methane emissions from the bison that occupied the Great Plains of North America before contact with European settlers. The study estimated that the removal of the bison caused a decrease of 2.2 Tg/yr. This is a proportionally large change for the time period.[36]

Another study examined the change of methane concentration in the atmosphere at the end of the Pleistocene epoch after the extinction of megafauna in the Americas. After early humans migrated to the Americas ~13,000 BP, their hunting and other associated ecological impacts led to the extinction of many megafaunal species in the region. Calculations suggest that this extinction decreased methane production by ~9.6 Tg/yr. Ice core records support this hypothesis of rapid methane decrease during the time period. This suggests that the absence of megafaunal methane emissions may have contributed to the abrupt climatic cooling at the onset of the Younger Dryas.[35]

[edit] Examples

The following are some notable examples of animals often considered as megafauna (in the sense of the "large animal" definition). This list is not intended to be exhaustive:

[edit] Gallery

[edit] Extinct

[edit] Living

[edit] See also

[edit] References

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  2. ^ a b Johnson, C. N. (2002-09-23). "Determinants of Loss of Mammal Species during the Late Quaternary 'Megafauna' Extinctions: Life History and Ecology, but Not Body Size". Proceedings of the Royal Society of London B (The Royal Society) 269 (1506): 2221–2227 (see p. 2225). doi:10.1098/rspb.2002.2130. JSTOR 3558643. 
  3. ^ Martin, P. S.; Steadman, D. W. (1999-06-30). "Prehistoric extinctions on islands and continents". In MacPhee, R. D. E. Extinctions in near time: causes, contexts and consequences. Advances in Vertebrate Paleontology. 2. New York: Kluwer/Plenum. pp. 17–56. ISBN 978-0306460920. OCLC 41368299. http://google.com/books?id=UZLuF1YXYTcC&pg=PA17. Retrieved 2011-08-23. 
  4. ^ Ice Age Animals. Illinois State Museum
  5. ^ a b c d e Evans, A. R.; et al. (2012-01-30). "The maximum rate of mammal evolution". PNAS 109. doi:10.1073/pnas.1120774109. http://www.pnas.org/content/early/2012/01/26/1120774109.abstract. Retrieved 2011-02-11. 
  6. ^ a b c d e f g Smith, F. A.; Boyer, A. G.; Brown, J. H.; Costa, D. P.; Dayan, T.; Ernest, S. K. M.; Evans, A. R.; Fortelius, M.; Gittleman, J. L.; Hamilton, M. J.; Harding, L. E.; Lintulaakso, K.; Lyons, S. K.; McCain, C.; Okie, J. G.; Saarinen, J. J.; Sibly, R. M.; Stephens, P. R.; Theodor, J.; Uhen, M. D. (2010-11-26). "The Evolution of Maximum Body Size of Terrestrial Mammals". Science 330 (6008): 1216-1219. doi:10.1126/science.1194830. http://www.sciencemag.org/content/330/6008/1216.short. Retrieved 2012-01-07. 
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  12. ^ Ibid. p. 212. http://google.com/books?id=-t6cQHdVEggC&pg=PA212. 
  13. ^ Ibid. p. 277. http://google.com/books?id=-t6cQHdVEggC&pg=PA277. 
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  22. ^ Norton, C. J.; Kondo, Y.; Ono, A.; Zhang, Y.; Diab, M. C. (2009-05-23). "The nature of megafaunal extinctions during the MIS 3–2 transition in Japan". Quaternary International 211 (1–2): 113–122. doi:10.1016/j.quaint.2009.05.002. http://www.sciencedirect.com/science/article/pii/S1040618209001451. Retrieved 2011-08-30. 
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