Calado Leandro, Cosenza Bernardo, Moraes Francisco, Dias Luko Caique, Mizrahi Damián, Xavier Fabio C, Batista Daniela, Domingos Roberto, Calazans Sávio, Araújo Fernanda, Coutinho Ricardo
Admiral Paulo Moreira Marine Research Institute (IEAPM), Brazilian Navy, Arraial do Cabo, 28930-000, Rio de Janeiro, Brazil.
Department of Oceanography, University of Rio de Janeiro State (UERJ), 20550-900, Brazil.
PLoS One. 2025 Jun 5;20(6):e0313240. doi: 10.1371/journal.pone.0313240. eCollection 2025.
The spread of invasive species in marine ecosystems is a growing global concern, particularly in regions with high economic and ecological importance. Sun corals (Tubastraea spp.) are native scleractinians from the Pacific Ocean that have spread along most of the Brazilian coast. This invasive species initially established populations in Rio de Janeiro state, SE Brazil, reaching high levels of abundance. Although the ecological aspects and impacts caused by this organism have been studied in detail, the natural mechanisms that drive its dispersal have attracted little attention. In this research, we focus on the coastal dispersion of sun coral larvae between Cabo de São Tomé and Ilha Grande Bay, and the offshore transport of sun coral larvae, investigating how submesoscale oceanographic features such as filaments, fronts and eddies influence connectivity among different sites. A high-resolution numerical model was used to simulate the coastal dynamics, incorporating the influence of the Brazil Current, wind-driven circulation, and submesoscale structures. Larval dispersal was examined under different wind scenarios, including northeasterly winds that drive southward currents and enhance offshore transport via submesoscale filaments. Results show that submesoscale features, particularly filaments emerged from upwelling regions, play a significant role on sun coral larvae dispersion. These features act as pathways that connect larvae from coastal to offshore oil exploration areas, highlighting the importance of both natural and anthropogenic processes for the dispersal of this invasive species. This research provides critical insights into the mechanisms governing the spread of invasive marine species, emphasizing the need for integrated coastal management strategies. Understanding how physical processes drive larval transport is essential for developing targeted control measures to mitigate the impact of invasive species like sun coral on native ecosystems and local economies. Furthermore, the study underscores the importance of monitoring both natural and anthropogenic influences on marine bioinvasions, particularly in regions with significant offshore industrial activities.
入侵物种在海洋生态系统中的扩散是一个日益引起全球关注的问题,尤其是在具有高度经济和生态重要性的地区。太阳珊瑚(Tubastraea spp.)是原产于太平洋的石珊瑚,已沿着巴西大部分海岸扩散。这种入侵物种最初在巴西东南部里约热内卢州建立种群,并达到了很高的丰度。尽管已经对这种生物的生态方面和造成的影响进行了详细研究,但驱动其扩散的自然机制却很少受到关注。在本研究中,我们聚焦于太阳珊瑚幼虫在圣多美角和大岛湾之间的海岸扩散以及太阳珊瑚幼虫的离岸运输,研究细丝、锋面和涡旋等次中尺度海洋学特征如何影响不同地点之间的连通性。使用高分辨率数值模型来模拟海岸动力学,纳入巴西暖流、风驱动环流和次中尺度结构的影响。在不同风况下检查幼虫扩散情况,包括驱动向南洋流并通过次中尺度细丝增强离岸运输的东北风。结果表明,次中尺度特征,特别是从上升流区域出现的细丝,在太阳珊瑚幼虫扩散中起重要作用。这些特征充当了将幼虫从沿海连接到近海石油勘探区域的通道,凸显了自然和人为过程对这种入侵物种扩散的重要性。本研究为控制入侵海洋物种扩散的机制提供了关键见解,并强调了综合海岸管理策略的必要性。了解物理过程如何驱动幼虫运输对于制定有针对性的控制措施以减轻太阳珊瑚等入侵物种对本地生态系统和地方经济的影响至关重要。此外,该研究强调了监测自然和人为因素对海洋生物入侵影响的重要性,特别是在具有重要近海工业活动的地区。