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两种线粒体分子标记指示的西沙太阳长棘海星(Acanthaster solaris)的扩散迁移

Dispersal and migration of Acanthaster solaris in Xisha Islands revealed by two mitochondrial molecular markers

  • 摘要: 本研究以西沙及鹿回头不同太阳长棘海星群体为研究对象,基于两种线粒体分子标记(COⅠ基因序列和线粒体控制区CR序列)测序分析,阐述了西沙及鹿回头不同岛礁太阳长棘海星的群体遗传结构、遗传多样性以及基因流情况。研究表明线粒体控制区CR序列多态性远高于COⅠ基因序列多态性,两种分子标记均揭示东岛多样性最高,鹿回头多样性最低,呈现从东南向西北逐渐减少的趋势。单倍型分析表明西沙及鹿回头太阳长棘海星均存在起源于一个原始单倍型的可能。与COⅠ序列单倍型相比,线粒体控制区CR序列单倍型在不同群体分布较为均匀。太阳长棘海星之间均存在至少一个从南向北的基因流方向,以及由西沙群岛海域中间向外迁移扩散,而相反方向基因流很小。上述结果为今后对西沙及鹿回头长棘海星暴发预测和管控提供理论支撑。

     

    Abstract: This study investigated the genetic structure, genetic diversity and gene flow of the Acanthaster solaris in Xisha Islands and Luhuitou, Hainan Island, using two mitochondrial molecular markers (COⅠ gene sequence and CR sequence in control area). Results showed that CR sequence polymorphism was much higher than COⅠ gene sequence polymorphism, and both markers indicated the highest genetic diversity in Dongdao Island and the lowest in Luhuitou, demonstrating a gradual decline in diversity from the southeast to the northwest. Haplotype analysis indicates that all A. solaris populations in both Xisha and Luhuitou may have originated from a single ancestral haplotype. Compared to COⅠ haplotypes, CR haplotypes were more evenly distributed across populations. There was at least one gene flow direction from south to north, as well as outward migration and diffusion from the central Xisha Islands, but the gene flow in the reverse-direction was minimal. These findings provide theoretical foundation for predicting and managing future outbreaks of A. solaris in Xisha Islands and Luhuitou region.

     

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