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Relative dating (''A'' was before ''B'') is often good enough for studying processes of evolution, but this has also been difficult, because of the problems involved in matching up rocks of the same age across different [[continent]]s, particularly around the internationally-defined [[Precambrian]]/[[Cambrian]] [[Global Boundary Stratotype Section and Point|boundary section]].<ref name=DatingProblems>e.g. {{Cite journal |
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| doi = 10.1017/S001675680100509X <!--Retrieved by bot--> |
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}}</ref> (the most common technique uses [[biostratigraphy| widespread but short-lived fossil species]] to identify rocks of similar ages) |
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So any dates or descriptions of sequences of events should be regarded with caution until better data become available. |
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==Types of evidence== |
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===Body fossils=== |
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Body fossils preserve significant parts of organisms and are therefore the most informative type of evidence. Unfortunately they are increasingly rare as one looks further back in time, among other reasons because the rocks in which they are buried are usually covered by more recent rocks and because they may have been [[erosion | eroded]] before being covered by later rocks. One recent study concluded that “parts of the fossil record are clearly incomplete, but they can be regarded as adequate to illustrate the broad patterns of the history of life.”<ref name="BentonQualityFossilRecord">{{cite journal |author=Benton MJ, Wills MA, Hitchin R |title=Quality of the fossil record through time |journal=Nature |volume=403 |issue=6769 |pages=534–7 |year=2000 |pmid=10676959 |doiFINDABLE =10.1038/35000558}}; Non-technical [http://palaeo.gly.bris.ac.uk/cladestrat/news.html summary]</ref> But there is evidence that some types of animals or parts of animals are relatively likely to be preserved as fossils in some environments and times, and extremely unlikely to be preserved in other environments and times. Part of this is due to changes in the chemistry of the oceans, which were partly caused by the on-going evolution of life, and these changes were most significant before the start of the Cambrian – for example any increase in the marine biomass would reduce the concentration of carbon, and the appearance of [[Porifera| sponges]] reduced the concentration of silicon.<ref name="Butterfield2003ExceptionalFossilPreservation">{{cite journal | author = Butterfield , N.J. | year =2003 | title = Exceptional Fossil Preservation and the Cambrian Explosion | journal = Integrative and Comparative Biology | volume = 43 | issue = 1 | pages = 166–177 | doiFINDABLE = 10.1093/icb/43.1.166 }}</ref> |
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Another limitation in the discovery and use of body fossils is the lack of preservation of large portions of the body. In most cases the sole anatomical features that are fossilized are the highly [[Mineralization|mineralised]] body parts containing high proportions of [[silica]] (sponges' skeletons), [[calcium carbonate]] (the shells of [[Bivalvia|bivalves]], [[Gastropoda|gastropods]] and [[ammonite]]s and [[exoskeleton]]s of most [[trilobite]]s and some [[crustacean]]s) or [[calcium phosphate]] (the [[bone]]s of [[vertebrate]]s). The majority of animal species living now are unlikely ever to leave fossils, since they are soft-bodied [[invertebrate]]s such as worms and slugs. Of the more than 30 [[phylum|phyla]] of living animals, two-thirds of these have never been found as fossils.<ref name ="CowenHistLife">{{ cite book | author=Cowen, R. | title=History of Life | publisher=Blackwell Science }}</ref> |
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[[Image:Marella200x155.png|thumb|200px|A fossil of ''[[Marrella]]'' from the [[Burgess Shale]] [[lagerstätte]]. The animal was under 2 cm long but the fine-grained shale has preserved a very detailed image of it.]] |
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The Cambrian fossil record includes an unusually high number of [[lagerstätte]]n which preserved the fossils' soft tissues in extremely fine detail, allowing a very informative study of animals that normally would not have left fossils. The fine detail of the deposits has allowed [[Paleontology|paleontologists]] to examine the internal workings of animals which in other sediments are only represented by shells, spines, claws, etc. The most significant Cambrian lagerstätten are: the early Cambrian [[Maotianshan shale]] beds of Chengjiang ([[Yunnan]], [[China]]) and [[Sirius Passet]] ([[Greenland]])<ref name=Morris1979>{{cite journal | author = Morris, S.C. | year = 1979 | title = The Burgess Shale (Middle Cambrian) Fauna | journal = Annual Review of Ecology and Systematics | volume = 10 | issue = 1 | pages = 327–349 | doiFINDABLE = 10.1146/annurev.es.10.110179.001551 }}</ref>; the middle Cambrian [[Burgess Shale]] ([[British Columbia]], [[Canada]])<ref name=Yochelson1996>{{cite journal | author = Yochelson, E.L. | year = 1996 | title = Discovery, Collection, and Description of the Middle Cambrian Burgess Shale Biota by Charles Doolittle Walcott | journal = Proceedings of the American Philosophical Society | volume = 140 | issue = 4 | pages = 469–545 | issn = | doiFINDABLE = | url = http://links.jstor.org/sici?sici=0003-049X(199612)140%3A4%3C469%3ADCADOT%3E2.0.CO%3B2-8 |
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| accessdate = 2007-04-24 }}</ref>; and the Upper Cambrian [[Orsten]] ([[Sweden]]) fossil beds. |
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While lagerstätten are superior to most fossil beds in preserving fine [[Anatomy|anatomical]] detail, they are far from perfect. The majority of then-living animals are probably not represented because lagerstätten are restricted to a narrow range of environments (e.g. where soft-bodied organisms can be preserved very quickly such as by mudslides), and the exceptional events that cause quick burial make it difficult to study the normal environments of the animals.<ref>{{cite journal | author = Butterfield, N.J. | year = 2001 | title = Ecology and evolution of Cambrian plankton | journal = The Ecology of the Cambrian Radiation. Columbia University Press, New York | pages = 200–216 | url = http://66.102.1.104/scholar?hl=en&lr=&ie=UTF-8&q=cache:9xeRu1SdF0QJ:www.earthscape.org/r3/ES14785/ch09.pdf+ | accessdate = 2007-08-19 |
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}}</ref> In addition, the known lagerstätten cover only a very limited period of time within the Cambrian, and none covers the crucial period just before the start of the Cambrian. Because normal fossil beds are very rare and lagerstätten even rarer, both are very unlikely to show the ''first'' occurrence of any type of organism.<ref name=Signor1982>{{cite journal | author = Signor, P.W. | year = 1982 | title = Sampling bias, gradual extinction patterns and catastrophes in the fossil record | journal = Geological implications of impacts of large asteroids and comets on the earth(A 84-25651 10-42). Boulder, CO, Geological Society of America, 1982, | pages = 291-296 | url = http://www.csa.com/partners/viewrecord.php?requester=gs&collection=TRD&recid=A8425675AH | accessdate = 2008-01-07}}</ref> |
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===Trace fossils=== |
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[[Image:Cruziana2.jpg|thumb|[[Trace fossil]] of the type called ''Cruziana'', possibly made by a [[trilobite]]. ]][[Trace fossils]] consist mainly of tracks and burrows on and under what was then the seabed. |
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Trace fossils are particularly significant because they represent a data source that is not limited to animals with easily-fossilized hard parts. Also many traces date from significantly earlier than the body fossils of animals that are thought to have been capable of making them.<ref name=Seilacher1994>e.g. {{cite journal |
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| author = Seilacher, A. |
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| year = 1994 |
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| title = How valid is Cruziana Stratigraphy? |
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| journal = International Journal of Earth Sciences |
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| volume = 83 |
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| issue = 4 |
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| pages = 752–758 |
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| url = http://www.springerlink.com/index/WP279834395100KH.pdf |
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| accessdate = 2007-09-09 |
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}}</ref> Whilst exact assignment of trace fossils to their makers is generally impossible, traces may provide the earliest physical evidence of the appearance of moderately complex animals (comparable to earthworms). |
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===Geochemical observations=== |
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The ratios of three major [[isotope analysis| isotopes]], <sup>87</sup>[[Strontium#Isotopes|Sr]] / <sup>86</sup>Sr, <sup>34</sup>[[Sulphur#Isotopes|S]] / <sup>32</sup>S and <sup>13</sup>[[Isotopes of carbon|C]] / <sup>12</sup>C, undergo dramatic fluctuations around the beginning of the Cambrian.<ref name=Magaritz1986>{{cite journal |
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| author = Magaritz, M. |
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| coauthors = Holser, W.T., Kirschvink, J.L. |
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| year = 1986 |
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| title = Carbon-isotope events across the Precambrian/Cambrian boundary on the Siberian Platform |
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| journal = Nature |
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| volume = 320 |
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| issue = 6059 |
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| pages = 258–259 |
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| issn = |
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| doiFINDABLE = 10.1038/320258a0 |
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| url = http://www.nature.com/nature/journal/v320/n6059/abs/320258a0.html |
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| accessdate = 2007-04-24 |
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}} |
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:Further documentation on these variations is available at the following URLs: [http://www.geol.umd.edu/~kaufman/pdf/Kaufman_95.pdf][http://www.geo.cornell.edu/geology/research/derry/publications/EPSL94.pdf][http://www.pnas.org/cgi/reprint/100/14/8124][http://www.journals.cambridge.org/download.php?file=%2FGEO%2FGEO135_04%2FS001675689800877Xa.pdf&code=ad7cfe63525b3a555d1724b76fbc7feb][http://www.journals.cambridge.org/download.php?file=%2FGEO%2FGEO134_01%2FS001675689700660Xa.pdf&code=ad7cfe63525b3a555367dab8427fc72d][http://arjournals.annualreviews.org/doi/pdf/10.1146/annurev.ea.22.050194.002125] (All listed at [http://scholar.google.com/scholar?hl=en&cites=584937827193315016&start=10 this Scholar results page]</ref> |
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This chemical signature in the rocks of the Precambrian/Cambrian boundary is difficult to interpret, and may be related to continental break-up, the end of a “[[snowball Earth|global glaciation]]”, or a catastrophic drop in productivity caused by a [[mass extinction]] just before the beginning of the Cambrian. |
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Carbon has 2 stable [[Isotopes of carbon| isotopes]], carbon-12 (<sup>12</sup>C) and carbon-13 (<sup>13</sup>C). Causes often suggested for changes in the ratio of <sup>13</sup>C to <sup>12</sup>C found in rocks include:<ref name="Marshall2006Explaining" /> |
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* A [[mass extinction]]. Chemistry is largely driven by electro-magnetic forces, and lighter isotopes such as <sup>12</sup>C respond to these more quickly than heavier ones such as <sup>13</sup>C. So living organisms generally contain a disproportionate amount of <sup>12</sup>C. A mass extinction would increase the amount of <sup>12</sup>C available to be included in rocks and therefore reduce the ratio of <sup>13</sup>C to <sup>12</sup>C. |
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* A [[Clathrate gun| methane “burp”]]. In [[Permafrost| permafrosts]] and [[continental shelves]] methane produced by [[Methanogen| bacteria]] gets trapped in “cages” of water molecules, forming a mixture called a [[methane clathrate| clathrate]]. This methane is very rich in <sup>12</sup>C because it has been produced by organisms. Clathrates may dissociate (break up) suddenly if the temperature rises or the pressure on them drops. Such dissociations release the <sup>12</sup>C-rich methane and thus reduce the ratio of <sup>13</sup>C to <sup>12</sup>C as this carbon is gradually incorporated into rocks (methane in the atmosphere breaks down into carbon dioxide and water; carbon dioxide reacts with minerals to form carbonate rocks). |
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===Comparative anatomy=== |
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[[Cladistics]] is a technique for working out the “family tree” of a set of organisms, and has most often applied to evidence from comparative anatomy (features of the bodies of organisms). In this kind of analysis it is possible to include both living and fossilized organisms and work out their evolutionary relationships. Sometimes one can conclude that group A must have evolved before groups B and C, because B and C have more similarities to each other than either has to A. On its own this method can say nothing about when A evolved, but if there are fossils of B or C dating from X million years ago, then A must have evolved more than X million years ago. |
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===Molecular phylogenetics=== |
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[[Molecular phylogenetics]] attempts to reconstruct the relationships between organisms by comparing details of their biochemistry, such as their [[DNA]]. In other words, it applies the analysis techniques of [[cladistics]] to biochemical rather than anatomical features. It provides an alternative line of evidence about evolution in the Cambrian and Precambrian, although the need for calibration against the fossil record means it is not entirely independent. Further, since the “clocks” measure molecular evolution, a period of rapid evolution is indistinguishable from a longer period of slow change, so it is unwise to rely on molecular phylogeny for estimates of dates<ref>L.A. Hug and A.J.Roger, The Impact of Fossils and Taxon Sampling on Ancient Molecular Dating Analyses. Molecular Biology and Evolution 2007 24(8):1889-1897, 2007</ref>. |
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Although this rapidly developing science must be treated with a degree of caution,<ref name=Ayala1999>{{cite journal | author = Ayala, F.J. | year = 1999 | title = Molecular clock mirages | journal = BioEssays | volume = 21 | issue = 1 | pages = 71–75 | doiFINDABLE = 10.1002/(SICI)1521-1878(199901)21:1%3C71::AID-BIES9%3E3.3.CO;2-2 |
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}}</ref> it has yielded some useful results. For example, it provides evidence that the three major animal groups diverged some time before the Cambrian, then independently underwent a rapid Cambrian diversification<ref name=De1999>{{cite journal | author = De Rosa, R. |
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| coauthors = Grenier, J.K.; Andreeva, T.; Cook, C.E.; Adoutte, A.; Akam, M.; Carroll, S.B.; Balavoine, G. | year = 1999 | title = Hox genes in brachiopods and priapulids and protostome evolution | journal = Nature | volume = 399 | issue = 6738 | pages = 772–776 | doiFINDABLE = 10.1038/21631 }}</ref> – although the reliability and implications of this apparent finding are still being debated.<ref name=Adoutte2000>{{cite journal | author = Adoutte, A. | coauthors = Balavoine, G.; Lartillot, N.; Lespinet, O.; Prud’homme, B.; De Rosa, R. |
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| year = 2000 | title = The new animal phylogeny: Reliability and implications | journal = PNAS | volume = 97 | issue = 9 | pages = 4453–4456 | url = http://cima.uprm.edu/~n_schizas/CMOB_8676/Adoutteetal2000.pdf |
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| accessdate = 2007-09-09 }}</ref> The current state of molecular phylogenetics seems not to support the Cambrian Explosion theory, but rather a considerably earlier [[evolutionary radiation]].<ref name="BlairHedges2004MolecularClocksDoNotSupportCambrianExplosion" /> |
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[[Trace fossils]] – broadly speaking, the traces made by organisms in the sediments they lived in or on – are of considerable importance in unravelling the Cambrian explosion. ''Bona fide'' burrows first appear in the Precambrian, from about {{Ma|555}} onwards;<ref name=Martin2000>{{cite journal |
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| author = Martin, M.W. |
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| coauthors = Grazhdankin, D.V.; Bowring, S.A.; Evans, D.A.D.; Fedonkin, M.A.; Kirschvink, J.L. |
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| year = 2000 |
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| date = [[2000-05-05]] |
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| title = Age of Neoproterozoic Bilatarian Body and Trace Fossils, White Sea, Russia: Implications for Metazoan Evolution |
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| journal = Science |
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| volume = 288 |
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| issue = 5467 |
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| pages = 841 |
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| issn = |
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| doiFINDABLE = 10.1126/science.288.5467.841 |
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| url = http://www.scienceonline.org/cgi/content/abstract/288/5467/841 |
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| accessdate = 2007-05-10 |
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}}</ref> at first, only simple horizontal burrows occur.<ref>{{cite book| |
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| title=Paleobiology of trace fossils |
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| author=Lockley, M.G. |
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| coauthor=Meyer, C.A., Hunt, A.P., Donovan, S. |
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| year=1994 |
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| publisher=Wiley and Sons |
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}}</ref> These marks were made by creatures moving across and below soft surfaces: the organisms making the traces were clearly not exploiting deep sediments, but only the topmost layers.<ref name=Seilacher1998>{{cite journal |
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| title=Animals More Than 1 Billion Years Ago: Trace Fossil Evidence from India |
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| author=Seilacher, A. |
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| authorlink=Adolf Seilacher |
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| coauthors=Bose, P.K. Pflüger, F. |
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| journal=Science |
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| volume=282 |
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| number=5386 |
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| pages=80–83 |
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| year=1998 |
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| url=http://sciencemag.org/cgi/content/full/282/5386/80 |
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| accessdate=2007-04-21 |
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}} |
}} |
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</ref> As the Cambrian got underway, new forms of trace fossil appeared, including vertical burrows<ref>e.g. ''[[Diplocraterion]]'' and ''[[Skolithos]]''</ref> and traces normally attributed to [[arthropod]]s.<ref>Such as ''[[Cruziana]]'' and ''[[Rusophycus]]''. Details of Cruziana’s formation |
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===Molluscs, annelids or brachiopods?=== |
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[[Image:halkieria2.jpg|thumb|150px|Fossil of ''[[Halkieria]] ]] |
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''[[Wiwaxia]]'', found so far only in the [[Burgess Shale]], had [[chitinous]] armor consisting of long vertical spines and short overlapping horizontal spines. It also had what looked like a [[radula]] (chitinous toothed “tongue”), a feature which is otherwise only known in molluscs. Some researchers think the pattern of its scales links its closely to the [[annelid]]s (worms) or more specifically to the [[polychaete]]s (“many bristles”; marine annelids with leg-like appendages); but others disagree.<ref>{{cite journal|author=Butterfield, N. J. |year=1990|title=A reassessment of the enigmatic Burgess Shale fossil ''Wiwaxia corrugata'' (Matthew) and its relationship to the polychaete ''Canadia spinosa'' (Walcott)|journal=Paleobiology|volume=16 |pages=287-303}}</ref><ref>{{cite journal|title=A reevaluation of Wiwaxia and the polychaetes of the Burgess Shale|author=Eibye-Jacobsen, D.|journal=Lethaia|volume=37|issue=3|pages=317-335|date=2004}}</ref> |
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''[[Orthrozanclus]]'', also discovered in the Burgess Shale, had long spines like those of the wiwaxiids, and small armor plates plus a cap of shell at the front end like those of the halkieriids. The scientists who described it say it may have been closely related to the halkieriids and the wiwaxiids.<ref>{{cite journal |
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| author =Conway Morris, S. and Caron, J-B. |
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| title =Halwaxiids and the Early Evolution of the Lophotrochozoans |
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| journal =Science |
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| volume =315 |
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| issue =5816 |
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| pages =1255-1258 |
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| date =2007 |
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| url =http://www.sciencemag.org/cgi/content/abstract/315/5816/1255 |
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}}</ref> |
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''[[Halkieria]]'' resembled a rather long slug, but had a small cap of shell at each end and overlapping armor plates covering the rest of its upper surface – the shell caps and armor plates were made of [[calcium carbonate]]. Its fossils are found on almost every continent in early to mid Cambrian deposits, and the “small shelly fauna” deposits contain many fragments which are now recognized as parts of ''Halkieria''’s armor. Some researchers have suggested that halkieriids were closely related to the ancestors of [[brachiopod]]s (the structure of halkieriids' front and rear shell caps resembles that of brachiopod shells) and to the wiwaxiids (the pattern of the scale armor over most of their bodies is very similar).<ref>{{cite journal |
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| last = |
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| first = |
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| author =Conway Morris, S. and Peel, J. S. |
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| title =Articulated Halkieriids from the Lower Cambrian of North Greenland and their Role in Early Protostome Evolution |
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| journal =Philosophical Transactions of the Royal Society: Biological Sciences |
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| volume =347 |
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| issue =1321 |
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| pages =305-358 |
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| date =1995 |
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| url =http://adsabs.harvard.edu/abs/1995RSPTB.347..305C |
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}}</ref> Others think the halkieriids are closely related to molluscs and have a particularly strong resemblance to [[chitons]].<ref>{{cite journal |
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| author =Vinther, J. and Nielsen, C. |
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| title = The Early Cambrian ''Halkieria'' is a mollusc |
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| journal =Zoologica Scripta |
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| volume =34 |
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| issue =1 |
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| pages =81-89 |
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| date =2005 |
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| url =http://www.ingentaconnect.com/content/bsc/zsc/2005/00000034/00000001/art00008;jsessionid=1jteckdcgr2to.alice |
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}}</ref> |
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''[[Odontogriphus]]'' is known from almost 200 specimens in the [[Burgess Shale]]. It was a flattened [[bilaterian]] up to 12 cm (5 in) long, oval in shape, with a ventral U-shaped mouth surrounded by small protrusions. The most recently found specimens are very well preserved and show what may be a radula, which led those who described these specimens to propose that it was a mollusc.<ref>{{cite journal |
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| author = Caron, J.B. |
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| coauthors = Scheltema, A.; Schander, C.; Rudkin, D. |
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| year = 2006 |
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| date=[[2006-07-13]] |
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| title = A soft-bodied mollusc with radula from the Middle Cambrian Burgess Shale |
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| journal = Nature |
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| volume = 442 |
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| issue = 7099 |
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| pages = 159–163 |
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| issn = |
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| doiFINDABLE = doi:10.1038/nature04894 |
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| url = http://www.nature.com/nature/journal/v442/n7099/pdf/nature04894.pdf |
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| accessdate = 2007-05-10 |
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}}</ref> But others disputed the finding of a radula and suggested ''Odontogriphus'' was a jawed segmented worm belonging to the [[Lophotrochozoa]] (a “super-phylum” which contains the annelids, brachiopods, molluscs and all other descendants of their last common ancestor).<ref name="Butterfield2006">{{cite journal |
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| author = Butterfield, N.J. |
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| year = 2006 |
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| title = Hooking some stem-group ‘‘worms’’: fossil lophotrochozoans in the Burgess Shale |
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| journal = Bioessays |
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| volume = 28 |
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| issue = 12 |
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| pages = 1161–1166 |
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| issn = |
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| doiFINDABLE = 10.1002/bies.20507 |
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| url = http://www3.interscience.wiley.com/cgi-bin/fulltext/113471993/PDFSTART |
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| accessdate = 2007-05-11 |
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}}</ref> |
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===Late Cambrian and early Ordovician organisms=== |
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[[Image:OilShaleFossilsEstonia.JPG|thumb| right | 200px | [[Bryozoa]]n fossils in an [[Ordovician]] [[oil shale]], northern [[Estonia]].]] |
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Right up to the end of the Cambrian there were high levels of “disparity” (sets of organisms with significantly different “designs”) but low levels of diversity (total numbers of species or [[genus| genera]]; variations on the main “design” themes); and as a result Cambrian ecosystems are much simpler than those from later in the [[Paleozoic]] era. There was a [[Cambrian-Ordovician extinction events| mass extinction]] at the Cambrian-Ordovician boundary, and typical Paleozoic marine diversity and ecosystems only appear during the recovery from the extinction.<ref name="Marshall2006Explaining" /> It is also worth noting that the earliest fossils of one [[phylum]], the [[Bryozoa]], first appear in the Ordovician period. |
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==Data from molecular phylogenetics== |
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A study in 1996 concluded that the genetic "family tree" of organisms indicates that [[protostomes]] (including the ancestors of molluscs, annelids and arthropods) diverged from [[deuterostomes]] (which includes the ancestors of chordates and echinoderms) about a billion years ago, almost twice as long ago as the start of the Cambrian; that, within the deuterostome group, [[chordates]] diverged from [[echinoderms]] some time later; and that the evolution of animal [[phylum | phyla]] was a long process.<ref name="WrayEtAl1996DeepPrecambrianDivergences">{{ cite journal | authors= Wray, G.A., Levinton, J.S., and Shapiro, L.H. | title=Molecular Evidence for Deep Precambrian Divergences Among Metazoan Phyla | journal=Science | date=October 1996 | volume=274 | issue=5287 | pages=568 - 573 | doiFINDABLE =10.1126/science.274.5287.568 | url=http://www.sciencemag.org/cgi/content/abstract/274/5287/568?rbfvrToken=f26c8ca37de67e0a3a66b56c414ba72393648832 }}</ref> A later study in 1998 found flaws in the first one and concluded that protostomes diverged from deuterostomes about 670M years ago and that chordates diverged from echinoderms about 600M years ago.<ref name="AyalaEtAl1998OriginOfMetazoanPhyla">{{ cite journal | authors=Ayala, F.J., Rzhetsky, A., and Ayala, F.J. | title=Origin of the metazoan phyla: Molecular clocks confirm paleontological estimates | journal=Proceeding of the National Academy of Sciences (of the USA) | volume=95 | issue=2 | pages=606-611 | date=January 1998 | url=http://www.pnas.org/cgi/content/abstract/95/2/606 }}</ref> |
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There is still debate about the interpretation of data from molecular phylogenetics. For example: one analysis in 2003 concluded that protostomes and deuterostomes diverged 582 ± 112 M years ago (note the wide margin of uncertainty; for example 582-112 = 470M years ago, after the ''end'' of the Cambrian);<ref name="ArisBrosouYang2003BayesianModelsOfEpisodicEvolution">{{ cite journal | authors=Aris-Brosou, S., and Yang, Z. | title=Bayesian Models of Episodic Evolution Support a Late Precambrian Explosive Diversification of the Metazoa | journal=Molecular Biology and Evolution | volume=20 | issue=12 | pages=1947-1954 | date=August 2003 | doiFINDABLE =10.1093/molbev/msg226 | url=http://mbe.oxfordjournals.org/cgi/content/abstract/20/12/1947?ijkey=488ce7b226719638ed13f71447a043a019c72fed&keytype2=tf_ipsecsha }}</ref> another in April 2004 concluded that the last common ancestor of [[bilaterians]] arose between 573M and 656M years ago, i.e. around the start of the [[Ediacaran]] period; <ref name="PetersonEtAl2004MetazoanDivergenceTimes">{{ cite journal | authors=Peterson, K.J., Lyons, J.B., Nowak, K.S., Takacs, C.M., Wargo, M.J., and McPeek, M.J. | title=Estimating metazoan divergence times with a molecular clock | journal=Proceeding of the National Academy of Sciences (of the USA) | date=April 2004 | volume=101 | issue=17 | pages=6536-6541 | doiFINDABLE =10.1073/pnas.0401670101 | url=http://www.pnas.org/cgi/content/abstract/101/17/6536?ijkey=6dfca1db78c568a083bf5a812f10bedd625bccd9&keytype2=tf_ipsecsha }}</ref> and a third in November 2004 concluded that the 2 previous ones was faulty and that protostomes and deuterostomes diverged 786M to 1,166M years ago, i.e. well before the start of the Ediacaran period.<ref name="BlairHedges2004MolecularClocksDoNotSupportCambrianExplosion">{{ cite journal | authors=Blair, J.E., and Hedges, S.B. | title=Molecular Clocks Do Not Support the Cambrian Explosion | journal=Molecular Biology and Evolution | volume=22 | issue=3 | pages=387-390 | doiFINDABLE =10.1093/molbev/msi039 | date=November 2004 | url=http://mbe.oxfordjournals.org/cgi/content/full/22/3/387#BIB2 }}</ref> |
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==How real was the explosion?== |
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===How fast did the main metazoan groups evolve?=== |
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In Darwin’s time what was known of the fossil record seemed to suggest that the major [[metazoan]] groups appeared in a few million years of the early to mid-Cambrian, and even in the 1980s this still appeared to be the case.<ref name="Whittington1985BurgessShale" /><ref name="WonderfulLife" /> But more recently-discovered fossil evidence suggests that at least some [[triploblastic]] [[bilaterians]] were present before the start of the Cambrian: ''[[Kimberella]]'' left the kind of fossils one would expect of an early mollusc, and the scratches on the rocks near these fossils suggest a mollusc-like method of feeding (555M years ago);<ref name="FedonkinWaggoner1997KimberellaMollusc" /> and if ''[[Vernanimalcula]]'' was a triploblastic bilaterian [[coelomate]], it would prove that moderately complex animals appeared even earlier (600-580M years ago).<ref name="Chen2004" /><ref name="Bengtson2004" /><ref name="ChenDefendVernanimacula" /> The presence of borings in shells of ''[[Cloudina]]'' suggests there were sufficiently advanced predators in the late [[Ediacaran]] period.<ref name="BengtsonZhao1992PredatorialBorings" /> Some mid-[[Ediacaran]] trace fossils appear to have been produced by animals more complex than [[flatworms]] and having [[hydrostatic skeleton]]s, about 565M years ago.<ref name="Erwin1999OriginOfBodyplans" /> |
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Further back in time, the long decline of [[stromatolites]] after about 1250 million years ago suggests that animals sufficiently complex to graze on bacterial mats were abundant well before the Ediacaran period;<ref name="McNamara1996DatingOriginAnimals" /> and the increase in abundance, diversity and spininess of acritarchs in the same period suggests that there were sufficient predators large enough to make such defenses necessary.<ref name="Bengtson2002OriginsOfPredation" /> |
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At the other end of the critical time range, several major modern types of animal did not appear until the late Cambrian, while typical Paleozoic ecosystems did not appear until the Ordovician.<ref name="Marshall2006Explaining" /> |
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So the evidence no longer appears to support the view that animals of "modern" complexity (comparable to living invertebrates) appeared in a few million years of the early to mid-Cambrian. But most modern [[phylum | phyla]] first appear in the Cambrian (except for possible molluscs, echinoderms and arthropods in the Ediacaran), and the rise in disparity (wide range of animals with significantly different "designs") seems to have occurred mostly in the early Cambrian.<ref name="Marshall2006Explaining" /> |
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===Was there a “riot of disparity” in the early Cambrian?=== |
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In this context “disparity” means a wide range of animals with significantly different “designs”; while “diversity” means total number of [[genus| genera]] or [[species]] and says nothing about the number of different basic “designs” (there ''could'' be many variations on the same few designs). There is little doubt that disparity rose sharply in the early Cambrian and was exceptionally high for the rest of the Cambrian – we see modern-looking animals such as [[crustaceans]], [[echinoderms]], and fish at about the same time and often in the same fossil beds as creatures like ''[[Anomalocaris]]'' and ''[[Halkieria]]'', which are currently regarded as “aunts” or “great-aunts” of modern groups.<ref name="Marshall2006Explaining" /> |
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On closer examination we find another surprise – some modern-looking animals, e.g. the early Cambrian crustaceans, [[trilobites]] and echinoderms, appear earlier in the fossil record than some of the “aunts” or “great-aunts” of modern groups.<ref name="ChenVannierHuang2001EarlyCrustaceans" /><ref name="SiveterWilliamsWaloszek2001Phosphatocopid" /><ref name="Lieberman1999Trilobites" /><ref name="DornbosBottjer2000Helicoplacoids" /> This could be a result of gaps in the fossil record or of preservational biases in different environments; or it could mean that the ancestors of various modern groups evolved at different times and possibly at different speeds.<ref name="Marshall2006Explaining" /> |
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==Possible causes of the “explosion”== |
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Despite the evidence that moderately complex animals ([[triploblastic]] [[bilaterians]]) existed before and possibly long before the start of the Cambrian, it seems that the pace of evolution was exceptionally fast in the early Cambrian. Naturally there has been a lot of discussion about why this should have happened. |
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===Changes in the environment=== |
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====Increase in oxygen levels==== |
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[[Earth's atmosphere| Earth’s earliest atmosphere]] contained no free [[oxygen]]; the oxygen that animals breathe today, both in the air and dissolved in water, is the product of billions of years of [[photosynthesis]], mainly by [[microorganisms]] such as [[cyanobacteria]]. The [[concentration]] of oxygen in the atmosphere has risen gradually (with a few ups and downs) over about the last 2.5 billion years (before that oxygen-hungry elements such as [[iron]] reacted with all the oxygen that was produced).<ref name ="CowenHistLife"/> |
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Shortage of oxygen might well have prevented the rise of large, complex animals for a long time. The amount of oxygen an animal can absorb is largely determined by the area of its oxygen-absorbing surfaces (lungs and gills in the most complex animals; the skin in less complex ones); but the amount needed is determined by its volume, which grows faster than the oxygen-absorbing area if an animal’s size increases equally in all directions. An increase in the concentration of oxygen in air or water would reduce or remove this difficulty. But apparently there was already enough oxygen to support reasonably large “[[Vendobionta]]” in the [[Ediacaran]] period.<ref name="Knoll1999" /> Perhaps a further increase in oxygen concentration was required to give animals the energy to produce substances such as [[collagen]] which are needed for the construction of complex structures, particularly those used in predation and defense against predation.<ref name=Towe1970>{{cite journal |
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| author = Towe, K.M. |
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| date = [[1970-04-01]] |
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| title = Oxygen-Collagen Priority and the Early Metazoan Fossil Record |
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| journal = Proceedings of the National Academy of Sciences |
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| volume = 65 |
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| issue = 4 |
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| pages = 781–788 |
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| doiFINDABLE = 10.1073/pnas.65.4.781 |
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| url=http://www.pnas.org/cgi/content/abstract/65/4/781 |
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}}</ref> |
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====Snowball Earths==== |
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There is plenty of evidence that in the late [[Neoproterozoic]] (extending into the early [[Ediacaran]] period) the Earth suffered [[Snowball Earth| massive glaciations]] in which most of its surface was covered by ice and temperatures were around freezing even at the [[Equator]]. Some researchers argue that these may have been an important factor in the Cambrian explosion, since the earliest known fossils of animals appear shortly after the last "Snowball Earth" episode.<ref name="HoffmanKaufman1998NeoproterozoicSnowball">{{ cite journal |
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| title=A Neoproterozoic Snowball Earth |
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| authors=Hoffman, P.F., Kaufman, A.J., Halverson, G.P., and Schrag, D.P. |
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| journal=Science |
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| date=28 August 1998 |
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| volume=281 |
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| issue=5381 |
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| pages=1342–1346 |
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| doiFINDABLE =10.1126/science.281.5381.1342 |
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| url=http://www.sciencemag.org/cgi/content/abstract/281/5381/1342 |
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}}</ref> |
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But it is hard to see how such catastrophes could have led to increases in the size and complexity of animals without clear evidence of a causal mechanism.<ref name="Marshall2006Explaining" /> Perhaps the cold temperatures increased the concentration of oxygen in the oceans—the [[solubility]] of oxygen nearly doubles as seawater cools from 30 °C to 0 °C.<ref name="RothmanHayesSummons2003NeoproterozoicCarbon">{{ cite journal |
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| title=Dynamics of the Neoproterozoic carbon cycle |
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| autoers=Rothman, D.H., Hayes, J.M., and Summons, R.E. |
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| journal=Proceedings of the National Academy of Sciences of the USA |
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| date=July 8 2003 |
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| volume=100 |
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| issue=14 |
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| pages=8124–8129 |
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| doiFINDABLE =10.1073/pnas.0832439100 |
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| publisher=The National Academy of Sciences |
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| url=http://www.pubmedcentral.nih.gov/articlerender.fcgi?artid=166193 |
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}}</ref> On the other hand they may have delayed the evolution of existing metazoans to larger sizes.<ref name="Bengtson2002OriginsOfPredation" /> |
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====Carbon isotope fluctuations==== |
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As we've already seen, there was a very sharp decrease in the <sup>13</sup>C/<sup>12</sup>C ratio at the Ediacaran-Cambrian boundary, followed by unusually strong fluctuations throughout the early Cambrian. Many scientists assume that the initial sharp drop represents a [[mass extinction]] at the start of the Cambrian.<ref name="Knoll1999" /><ref name="Amthor2003" /> It might even have caused a mass extinction – the [[Permian–Triassic extinction event]] is associated with a similar sharp |
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decrease in the <sup>13</sup>C/<sup>12</sup>C ratio; this is usually explained as due to massive dissociation of [[methane clathrates]], and it is widely thought that the resulting methane emissions triggered severe global warming and other environmental catastrophes. And the <sup>13</sup>C/<sup>12</sup>C fluctuations in the early Cambrian resemble those of the early [[Triassic]], when life was struggling to recover from the Permian-Triassic extinction.<ref name="">{{ cite journal |
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| authors=Payne, J.L., Lehrmann, D.J., Jiayong, W., Orchard, M.J., Schrag, D.P., and Knoll, A.H. |
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| date=23 July 2004 |
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Large perturbations of the Carbon cycle during recovery from the end-Permian extinction |
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| journal=Science |
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| volume=305 |
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| issue=5683 |
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| pages=506–509 |
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| doiFINDABLE =10.1126/science.1097023 |
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| url=http://www.sciencemag.org/cgi/content/abstract/305/5683/506?ijkey=f1abe74c48d1cdf246ea6c1bf19420a2c2c00d3d&keytype2=tf_ipsecsha |
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}}</ref> |
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But it’s difficult to see how a mass extinction could have triggered a sharp increase in disparity and diversity. Mass extinctions such as the Permian-Triassic and [[Cretaceous–Tertiary extinction event| Cretaceous–Tertiary]] raised ''existing'' animals from insignificance to “dominance”, but these replaced different but similarly complex animals that were dominant before these extinctions, and there was no increase in disparity or diversity.<ref name="Marshall2006Explaining" /> |
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Others have suggested that each short-term decrease in the <sup>13</sup>C/<sup>12</sup>C ratio through out the early Cambrian represents a methane “burp” which, by raising global temperatures, triggered an increase in diversity.<ref name="KirschvinkRaub2003Methane Fuse">{{cite journal |
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| authors=Kirschvink, J.L., and Raub, T.D. |
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| title=A methane fuse for the Cambrian explosion: carbon cycles and true polar wander |
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| journal=Comptes Rendus Geosciences |
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| volume=335 |
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| issue=1 |
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| date=January 2003 |
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| pages=65–78 |
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| doiFINDABLE =10.1016/S1631-0713(03)00011-7 |
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| url=http://www.gps.caltech.edu/~jkirschvink/pdfs/KirschvinkRaubComptesRendus.pdf |
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}}</ref> But this hypothesis also fails explain the increase in ''disparity''.<ref name="Marshall2006Explaining" /> |
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===Developmental Explanations=== |
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Some theories are based on the idea that relatively small changes in the way in which animals develop from [[embryo]] to adult may have produced very rapid evolution of body forms. Unfortunately such theories do not explain why the origin of such a development system should by itself lead to increased diversity or disparity. In fact if at least one [[Ediacaran biota| Ediacaran]] is a [[bilaterian]] (for example ''[[Kimberella]]'', ''[[Spriggina]]'' or ''[[Arkarua]]''), then the bilaterian developmental system |
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==References== |
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{{reflist|2}} |
Revision as of 20:55, 12 March 2008
Relative dating (A was before B) is often good enough for studying processes of evolution, but this has also been difficult, because of the problems involved in matching up rocks of the same age across different continents, particularly around the internationally-defined Precambrian/Cambrian boundary section.[1] (the most common technique uses widespread but short-lived fossil species to identify rocks of similar ages)
So any dates or descriptions of sequences of events should be regarded with caution until better data become available.
Types of evidence
Body fossils
Body fossils preserve significant parts of organisms and are therefore the most informative type of evidence. Unfortunately they are increasingly rare as one looks further back in time, among other reasons because the rocks in which they are buried are usually covered by more recent rocks and because they may have been eroded before being covered by later rocks. One recent study concluded that “parts of the fossil record are clearly incomplete, but they can be regarded as adequate to illustrate the broad patterns of the history of life.”[2] But there is evidence that some types of animals or parts of animals are relatively likely to be preserved as fossils in some environments and times, and extremely unlikely to be preserved in other environments and times. Part of this is due to changes in the chemistry of the oceans, which were partly caused by the on-going evolution of life, and these changes were most significant before the start of the Cambrian – for example any increase in the marine biomass would reduce the concentration of carbon, and the appearance of sponges reduced the concentration of silicon.[3]
Another limitation in the discovery and use of body fossils is the lack of preservation of large portions of the body. In most cases the sole anatomical features that are fossilized are the highly mineralised body parts containing high proportions of silica (sponges' skeletons), calcium carbonate (the shells of bivalves, gastropods and ammonites and exoskeletons of most trilobites and some crustaceans) or calcium phosphate (the bones of vertebrates). The majority of animal species living now are unlikely ever to leave fossils, since they are soft-bodied invertebrates such as worms and slugs. Of the more than 30 phyla of living animals, two-thirds of these have never been found as fossils.[4]
The Cambrian fossil record includes an unusually high number of lagerstätten which preserved the fossils' soft tissues in extremely fine detail, allowing a very informative study of animals that normally would not have left fossils. The fine detail of the deposits has allowed paleontologists to examine the internal workings of animals which in other sediments are only represented by shells, spines, claws, etc. The most significant Cambrian lagerstätten are: the early Cambrian Maotianshan shale beds of Chengjiang (Yunnan, China) and Sirius Passet (Greenland)[5]; the middle Cambrian Burgess Shale (British Columbia, Canada)[6]; and the Upper Cambrian Orsten (Sweden) fossil beds.
While lagerstätten are superior to most fossil beds in preserving fine anatomical detail, they are far from perfect. The majority of then-living animals are probably not represented because lagerstätten are restricted to a narrow range of environments (e.g. where soft-bodied organisms can be preserved very quickly such as by mudslides), and the exceptional events that cause quick burial make it difficult to study the normal environments of the animals.[7] In addition, the known lagerstätten cover only a very limited period of time within the Cambrian, and none covers the crucial period just before the start of the Cambrian. Because normal fossil beds are very rare and lagerstätten even rarer, both are very unlikely to show the first occurrence of any type of organism.[8]
Trace fossils

Trace fossils consist mainly of tracks and burrows on and under what was then the seabed.
Trace fossils are particularly significant because they represent a data source that is not limited to animals with easily-fossilized hard parts. Also many traces date from significantly earlier than the body fossils of animals that are thought to have been capable of making them.[9] Whilst exact assignment of trace fossils to their makers is generally impossible, traces may provide the earliest physical evidence of the appearance of moderately complex animals (comparable to earthworms).
Geochemical observations
The ratios of three major isotopes, 87Sr / 86Sr, 34S / 32S and 13C / 12C, undergo dramatic fluctuations around the beginning of the Cambrian.[10] This chemical signature in the rocks of the Precambrian/Cambrian boundary is difficult to interpret, and may be related to continental break-up, the end of a “global glaciation”, or a catastrophic drop in productivity caused by a mass extinction just before the beginning of the Cambrian.
Carbon has 2 stable isotopes, carbon-12 (12C) and carbon-13 (13C). Causes often suggested for changes in the ratio of 13C to 12C found in rocks include:[11]
- A mass extinction. Chemistry is largely driven by electro-magnetic forces, and lighter isotopes such as 12C respond to these more quickly than heavier ones such as 13C. So living organisms generally contain a disproportionate amount of 12C. A mass extinction would increase the amount of 12C available to be included in rocks and therefore reduce the ratio of 13C to 12C.
- A methane “burp”. In permafrosts and continental shelves methane produced by bacteria gets trapped in “cages” of water molecules, forming a mixture called a clathrate. This methane is very rich in 12C because it has been produced by organisms. Clathrates may dissociate (break up) suddenly if the temperature rises or the pressure on them drops. Such dissociations release the 12C-rich methane and thus reduce the ratio of 13C to 12C as this carbon is gradually incorporated into rocks (methane in the atmosphere breaks down into carbon dioxide and water; carbon dioxide reacts with minerals to form carbonate rocks).
Comparative anatomy
Cladistics is a technique for working out the “family tree” of a set of organisms, and has most often applied to evidence from comparative anatomy (features of the bodies of organisms). In this kind of analysis it is possible to include both living and fossilized organisms and work out their evolutionary relationships. Sometimes one can conclude that group A must have evolved before groups B and C, because B and C have more similarities to each other than either has to A. On its own this method can say nothing about when A evolved, but if there are fossils of B or C dating from X million years ago, then A must have evolved more than X million years ago.
Molecular phylogenetics
Molecular phylogenetics attempts to reconstruct the relationships between organisms by comparing details of their biochemistry, such as their DNA. In other words, it applies the analysis techniques of cladistics to biochemical rather than anatomical features. It provides an alternative line of evidence about evolution in the Cambrian and Precambrian, although the need for calibration against the fossil record means it is not entirely independent. Further, since the “clocks” measure molecular evolution, a period of rapid evolution is indistinguishable from a longer period of slow change, so it is unwise to rely on molecular phylogeny for estimates of dates[12].
Although this rapidly developing science must be treated with a degree of caution,[13] it has yielded some useful results. For example, it provides evidence that the three major animal groups diverged some time before the Cambrian, then independently underwent a rapid Cambrian diversification[14] – although the reliability and implications of this apparent finding are still being debated.[15] The current state of molecular phylogenetics seems not to support the Cambrian Explosion theory, but rather a considerably earlier evolutionary radiation.[16]
- ^ e.g. Gehling, James; Jensen, Sören; Droser, Mary; Myrow, Paul; Narbonne, Guy (March 2001). "Burrowing below the basal Cambrian GSSP, Fortune Head, Newfoundland". Geological Magazine. 138 (2): 213–218.
{{cite journal}}
: Unknown parameter|doiFINDABLE=
ignored (help)CS1 maint: date and year (link) - ^ Benton MJ, Wills MA, Hitchin R (2000). "Quality of the fossil record through time". Nature. 403 (6769): 534–7. PMID 10676959.
{{cite journal}}
: Unknown parameter|doiFINDABLE=
ignored (help)CS1 maint: multiple names: authors list (link); Non-technical summary - ^ Butterfield , N.J. (2003). "Exceptional Fossil Preservation and the Cambrian Explosion". Integrative and Comparative Biology. 43 (1): 166–177.
{{cite journal}}
: Unknown parameter|doiFINDABLE=
ignored (help) - ^ Cowen, R. History of Life. Blackwell Science.
- ^ Morris, S.C. (1979). "The Burgess Shale (Middle Cambrian) Fauna". Annual Review of Ecology and Systematics. 10 (1): 327–349.
{{cite journal}}
: Unknown parameter|doiFINDABLE=
ignored (help) - ^ Yochelson, E.L. (1996). "Discovery, Collection, and Description of the Middle Cambrian Burgess Shale Biota by Charles Doolittle Walcott". Proceedings of the American Philosophical Society. 140 (4): 469–545. Retrieved 2007-04-24.
{{cite journal}}
: Cite has empty unknown parameter:|doiFINDABLE=
(help) - ^ Butterfield, N.J. (2001). "Ecology and evolution of Cambrian plankton". The Ecology of the Cambrian Radiation. Columbia University Press, New York: 200–216. Retrieved 2007-08-19.
- ^ Signor, P.W. (1982). "Sampling bias, gradual extinction patterns and catastrophes in the fossil record". Geological implications of impacts of large asteroids and comets on the earth(A 84-25651 10-42). Boulder, CO, Geological Society of America, 1982,: 291–296. Retrieved 2008-01-07.
{{cite journal}}
: CS1 maint: extra punctuation (link) - ^ e.g. Seilacher, A. (1994). "How valid is Cruziana Stratigraphy?" (PDF). International Journal of Earth Sciences. 83 (4): 752–758. Retrieved 2007-09-09.
- ^ Magaritz, M. (1986). "Carbon-isotope events across the Precambrian/Cambrian boundary on the Siberian Platform". Nature. 320 (6059): 258–259. Retrieved 2007-04-24.
{{cite journal}}
: Unknown parameter|coauthors=
ignored (|author=
suggested) (help); Unknown parameter|doiFINDABLE=
ignored (help) - ^ Cite error: The named reference
Marshall2006Explaining
was invoked but never defined (see the help page). - ^ L.A. Hug and A.J.Roger, The Impact of Fossils and Taxon Sampling on Ancient Molecular Dating Analyses. Molecular Biology and Evolution 2007 24(8):1889-1897, 2007
- ^ Ayala, F.J. (1999). "Molecular clock mirages". BioEssays. 21 (1): 71–75.
{{cite journal}}
: Unknown parameter|doiFINDABLE=
ignored (help) - ^ De Rosa, R. (1999). "Hox genes in brachiopods and priapulids and protostome evolution". Nature. 399 (6738): 772–776.
{{cite journal}}
: Unknown parameter|coauthors=
ignored (|author=
suggested) (help); Unknown parameter|doiFINDABLE=
ignored (help) - ^ Adoutte, A. (2000). "The new animal phylogeny: Reliability and implications" (PDF). PNAS. 97 (9): 4453–4456. Retrieved 2007-09-09.
{{cite journal}}
: Unknown parameter|coauthors=
ignored (|author=
suggested) (help) - ^ Cite error: The named reference
BlairHedges2004MolecularClocksDoNotSupportCambrianExplosion
was invoked but never defined (see the help page).
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