Purser Autun, Herr Helena, Dreutter Simon, Dorschel Boris, Glud Ronnie N, Hehemann Laura, Hoge Ulrich, Jamieson Alan J, Linley Thomas D, Stewart Heather A, Wenzhöfer Frank
Alfred Wegener Helmholz Institute of Polar and Marine Research, Bremerhaven, Germany.
Center of Natural History, University of Hamburg, Hamburg, Germany.
R Soc Open Sci. 2019 Mar 13;6(3):182053. doi: 10.1098/rsos.182053. eCollection 2019 Mar.
This comment presents acoustic and visual data showing deep seafloor depression chains similar to those reported in Marsh ( 5: 180286), though from a different deep-sea setting. Marsh present data collected during cruise JC120 from polymetallic nodule rich sites within the Clarion-Clipperton Fracture Zone (CCFZ), at water depths of between 3999 and 4258 m. Within this comment, we present data collected with equivalent acoustic and imaging devices on-board the RV Sonne (SO261-March/April 2018) from the Atacama Trench, approximately 4000 m depth, which shows comparable depression chains in the seafloor. In contrast with the CCFZ observations, our study area was wholly free of polymetallic nodules, an observation therefore weakening the 'ballast collection' by deep-sea diving mammals formation hypothesis discussed in their paper We support their alternate hypothesis that if these features are indeed generated by deep-diving megafauna, then they are more likely the resultant traces of infauna feeding or marks made during opportunistic capture of benthic fish/cephalopods. We observed these potential prey fauna with lander and towed camera systems during the cruise, with example images of these presented here. Both the SO261 and JC120 cruises employed high-resolution sidescan systems at deployment altitudes seldom used routinely until the last few years during scientific deep-sea surveys. Given that both cruises found these depression chains in contrasting physical regions of the East Pacific, they may have a more ubiquitous distribution than at just these sites. Thus, the impacts of cetacean foraging behaviour on deep seafloor communities, and the potential relevance of these prey sources to deep-diving species, should be considered.
本评论展示了声学和视觉数据,这些数据显示出与Marsh(5: 180286)报道的类似的深海海底凹陷链,不过是来自不同的深海环境。Marsh展示了在巡航JC120期间从克拉里昂-克利珀顿断裂带(CCFZ)内富含多金属结核的站点收集的数据,水深在3999米至4258米之间。在本评论中,我们展示了在RV Sonne号船上(2018年3月/4月,SO261)使用等效声学和成像设备从阿塔卡马海沟(深度约4000米)收集的数据,该数据显示出海底有类似的凹陷链。与CCFZ的观测结果不同,我们的研究区域完全没有多金属结核,因此这一观测结果削弱了他们论文中讨论的深海潜水哺乳动物形成“压载物收集”的假说。我们支持他们的另一种假说,即如果这些特征确实是由深潜大型动物群产生的,那么它们更有可能是底栖动物觅食的痕迹,或者是在机会性捕获底栖鱼类/头足类动物时留下的印记。在巡航期间,我们使用着陆器和拖曳式摄像系统观测到了这些潜在的猎物动物群,此处展示了它们的示例图像。SO26仁号和JC120号巡航都采用了高分辨率侧扫系统,其部署高度在过去几年科学深海调查中很少常规使用。鉴于这两次巡航都在东太平洋不同的物理区域发现了这些凹陷链,它们的分布可能比仅在这些站点更为普遍。因此,应该考虑鲸类觅食行为对深海海底群落的影响,以及这些猎物来源与深潜物种的潜在相关性。