Waters Jonathan M, Roy Michael S
Department of Zoology, University of Otago, P.O. Box 56, Dunedin, New Zealand.
Syst Biol. 2004 Feb;53(1):18-24. doi: 10.1080/10635150490264671.
We used mitochondrial DNA (mtDNA) sequences to test biogeographic hypotheses for Patiriella exigua (Asterinidae), one of the world's most widespread coastal sea stars. This small intertidal species has an entirely benthic life history and yet occurs in southern temperate waters of the Atlantic, Indian, and Pacific oceans. Despite its abundance around southern Africa, southeastern Australia, and several oceanic islands, P. exigua is absent from the shores of Western Australia, New Zealand, and South America. Phylogenetic analysis of mtDNA sequences (cytochrome oxidase I, control region) indicates that South Africa houses an assemblage of P. exigua that is not monophyletic (P = 0.04), whereas Australian and Lord Howe Island specimens form an interior monophyletic group. The placement of the root in Africa and small genetic divergences between eastern African and Australian haplotypes strongly suggest Pleistocene dispersal eastward across the Indian Ocean. Dispersal was probably achieved by rafting on wood or macroalgae, which was facilitated by the West Wind Drift. Genetic data also support Pleistocene colonization of oceanic islands (Lord Howe Island, Amsterdam Island, St. Helena). Although many biogeographers have speculated about the role of long-distance rafting, this study is one of the first to provide convincing evidence. The marked phylogeographic structure evident across small geographic scales in Australia and South Africa indicates that gene flow among populations may be generally insufficient to prevent the local evolution of monophyly. We suggest that P. exigua may rely on passive mechanisms of dispersal.
我们利用线粒体DNA(mtDNA)序列来检验细纹盘海星(Asterinidae)的生物地理学假说,细纹盘海星是世界上分布最广的沿海海星之一。这种小型潮间带物种具有完全底栖的生活史,却出现在大西洋、印度洋和太平洋的南温带水域。尽管细纹盘海星在非洲南部、澳大利亚东南部和一些海洋岛屿周围数量众多,但在西澳大利亚、新西兰和南美洲的海岸却没有。对mtDNA序列(细胞色素氧化酶I、控制区)的系统发育分析表明,南非的细纹盘海星群体并非单系群(P = 0.04),而澳大利亚和豪勋爵岛的标本形成一个内部单系群。根部位于非洲以及东非和澳大利亚单倍型之间较小的遗传差异强烈表明,更新世时期该物种通过印度洋向东扩散。扩散可能是通过附着在木材或大型藻类上漂流实现的,西风漂流促进了这种漂流。遗传数据也支持该物种在更新世时期对海洋岛屿(豪勋爵岛、阿姆斯特丹岛、圣赫勒拿岛)的殖民。尽管许多生物地理学家推测过远距离漂流的作用,但这项研究是最早提供令人信服证据的研究之一。在澳大利亚和南非小地理尺度上明显的显著系统地理结构表明,种群间的基因流动可能通常不足以阻止单系群的局部进化。我们认为细纹盘海星可能依赖被动扩散机制。