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掠食性海星幼体在保育栖息地的等待阶段

The Waiting Stage, Prolonged Residency in Nursery Habitats by Juveniles of the Predatory Sea Star .

出版信息

Biol Bull. 2021 Dec;241(3):219-230. doi: 10.1086/715843. Epub 2021 Nov 16.

Abstract

AbstractGrowth and recruitment of the sea star was followed over six years in Lough Hyne, southwest Ireland. Juveniles from a 2-mm radius were found on algae at <1-2-m depth following what appeared to be gregarious larval settlement. Data from Lough Hyne and Mulroy Bay (northwest Ireland) indicated that algal habitat serves as a nursery area for juveniles of . Successive size frequency modes of the juveniles at Lough Hyne indicated slow growth over 6 years, to a mean radius of 20 mm. The absence of additional recruitment allowed monitoring of a discrete population. Recruits in the nursery habitat over the six years remained as waiting stage juveniles, a Peter Pan group with delayed maturity subsisting on a diet of epibionts. An initial sharp decline in numbers indicated post-settlement mortality, with subsequent decline likely due to migration to the adjacent shelly habitat, where subadult (30-70-mm radius) lives. In this habitat, preys on small bivalves and eventually joins the adult (maximum radius = 280 mm) population on open sediment, where it feeds on large bivalves. Size frequency distributions of the juveniles and adults showed growth over the six years, with the waiting stage sea stars slowly merging in size with the adult population. It appears that the supply of new individuals into the adult population may take place six or more years following settlement. Strong connectivity between life stage habitats and prolonged recruitment into the adult population may contribute to balanced exploitation of infaunal prey.

摘要

摘要

在爱尔兰西南部的 Lough Hyne,我们对海星的生长和补充种群进行了六年多的跟踪研究。在 1-2 米深的藻类上发现了半径为 2 毫米的幼体,这表明幼虫似乎是群居定居的。来自 Lough Hyne 和 Mulroy Bay(爱尔兰西北部)的数据表明,藻类生境是幼体的育幼区。Lough Hyne 幼体的连续大小频率模式表明,6 年来生长缓慢,平均半径为 20 毫米。由于没有额外的补充种群,因此可以监测到一个离散的种群。六年来,育幼区的补充幼体仍然处于等待成熟阶段的幼体,是一个彼得潘群体,成熟延迟,以附生生物为食。最初数量的急剧下降表明了定居后的死亡率,随后的下降可能是由于迁移到相邻的有壳生境,那里有亚成体(半径 30-70 毫米)居住。在这个生境中,以小型双壳类动物为食,最终加入成年(最大半径=280 毫米)种群,在开放的沉积物上以大型双壳类动物为食。幼体和成年体的大小频率分布表明,在六年中都有生长,等待成熟阶段的海星的大小与成年种群逐渐趋同。看来,新个体进入成年种群的供应可能在定居后六年或更长时间发生。生命阶段栖息地之间的强连接和对成年种群的长期补充可能有助于平衡利用底栖猎物。

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