Biol Bull. 2021 Dec;241(3):271-285. doi: 10.1086/717539. Epub 2021 Nov 19.
AbstractPopulation irruptions of the western Pacific crown-of-thorns sea star ( sp.) are a perennial threat to coral reefs and may be initiated by fluctuations in reproductive or settlement success. However, the processes dictating their early life history, particularly larval settlement, remain poorly understood given limitations in sampling larvae and newly settled juveniles in the field. Here, we introduce an innovative method to measure crown-of-thorns sea star settlement, using artificial settlement collectors and droplet digital polymerase chain reaction based on crown-of-thorns sea star-specific mitochondrial DNA primers. This study demonstrated the utility of this method and explored temporal and spatial patterns of crown-of-thorns sea star settlement on the Great Barrier Reef from 2016 to 2020. Settlement varied considerably between sampling periods at Rib Reef and peaked between October 2016 and January 2017. Our results further suggest that crown-of-thorns sea star larvae readily settle in shallow reef environments, with no preferential settlement detected between depths tested (4-12 m). Substantial variation between Great Barrier Reef regions was revealed in 2019-2020, because collectors deployed on reefs in the central Great Barrier Reef were >10 times as likely to record newly settled crown-of-thorns sea stars as reefs in the northern Great Barrier Reef near Lizard Island. The trends reported here add to our understanding of this critical life-history stage; however, further method validation and larger-scale studies are needed to address pertinent information gaps, such as the stock-recruitment dynamics of this species. Most importantly, fluctuations in crown-of-thorns sea star settlement can now be detected using this sampling protocol, which demonstrates its utility in heralding new and renewed population irruptions of this destructive sea star.
西太平洋棘冠海星(Sp.)的种群爆发是珊瑚礁的常年威胁,可能是由繁殖或定居成功率的波动引发的。然而,由于在野外对幼虫和新定居的幼体进行采样的限制,它们早期生活史的过程,特别是幼虫定居,仍然知之甚少。在这里,我们介绍了一种使用人工定居收集器和基于棘冠海星特异性线粒体 DNA 引物的液滴数字聚合酶链反应来测量棘冠海星定居的创新方法。本研究证明了该方法的实用性,并探讨了 2016 年至 2020 年大堡礁上棘冠海星定居的时空模式。在里布礁的采样期间,定居情况差异很大,2016 年 10 月至 2017 年 1 月达到峰值。我们的结果进一步表明,棘冠海星幼虫很容易在浅礁环境中定居,在测试的深度(4-12 米)之间没有发现优先定居。2019-2020 年,大堡礁地区之间存在很大差异,因为在大堡礁中部部署的收集器记录到新定居的棘冠海星的可能性是蜥蜴岛附近大堡礁北部的珊瑚礁的 10 倍以上。这里报告的趋势增加了我们对这个关键生活史阶段的理解;然而,需要进一步的方法验证和更大规模的研究来解决相关的信息差距,例如该物种的种群补充动态。最重要的是,现在可以使用这种采样方案检测棘冠海星定居的波动,这证明了它在预示这种破坏性海星新的和新的种群爆发方面的实用性。