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The term "clade" was coined in 1957 by the biologist Julian Huxley to refer to the result of cladogenesis, a concept Huxley borrowed from Bernhard Rensch.[1][2]
A clade is by definition population, or a species) and all its descendants.[note 1][3][4] The ancestor can be known or unknown; any and all members of a clade can be extant or extinct.
The science that tries to reconstruct phylogenetic trees and thus discover clades is called phylogenetics or cladistics, the latter term being derived from "clade" by Ernst Mayr (1965). The results of phylogenetic/cladistic analyses are tree-shaped diagrams called cladograms; they, and all their branches, are phylogenetic hypotheses.[5]
Three methods of defining clades are featured in phylogenetic nomenclature: node-, stem-, and apomorphy-based (see here for detailed definitions).
The relationship between clades can be described in several ways:
The idea of a clade did not exist in pre-Systema Naturae (notably among the vertebrate groups) do represent clades. The phenomenon of convergent evolution is however responsible for many cases where there are misleading similarities in the morphology of groups that evolved from different lineages.
With the publication of Darwin's theory of evolution in 1859, the idea was born that groups used in a system of classification should represent branches on the evolutionary tree of life. In the century and a half since then, taxonomists have increasingly worked to make the taxonomic system reflect evolution. When it comes to naming, however, this principle is not always compatible with the traditional rank-based nomenclature. In the latter, only taxa associated with a rank can be named, yet there are not enough ranks to name a long series of nested clades; also, taxon names cannot be defined in a way that guarantees them to refer to clades. For these and other reasons, phylogenetic nomenclature has been developed; it is still controversial.
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