Hewson Ian, Button Jason B, Gudenkauf Brent M, Miner Benjamin, Newton Alisa L, Gaydos Joseph K, Wynne Janna, Groves Cathy L, Hendler Gordon, Murray Michael, Fradkin Steven, Breitbart Mya, Fahsbender Elizabeth, Lafferty Kevin D, Kilpatrick A Marm, Miner C Melissa, Raimondi Peter, Lahner Lesanna, Friedman Carolyn S, Daniels Stephen, Haulena Martin, Marliave Jeffrey, Burge Colleen A, Eisenlord Morgan E, Harvell C Drew
Department of Microbiology, Cornell University, Ithaca, NY 14853;
Department of Biology, Western Washington University, Bellingham, WA 98225;
Proc Natl Acad Sci U S A. 2014 Dec 2;111(48):17278-83. doi: 10.1073/pnas.1416625111. Epub 2014 Nov 17.
Populations of at least 20 asteroid species on the Northeast Pacific Coast have recently experienced an extensive outbreak of sea-star (asteroid) wasting disease (SSWD). The disease leads to behavioral changes, lesions, loss of turgor, limb autotomy, and death characterized by rapid degradation ("melting"). Here, we present evidence from experimental challenge studies and field observations that link the mass mortalities to a densovirus (Parvoviridae). Virus-sized material (i.e., <0.2 μm) from symptomatic tissues that was inoculated into asymptomatic asteroids consistently resulted in SSWD signs whereas animals receiving heat-killed (i.e., control) virus-sized inoculum remained asymptomatic. Viral metagenomic investigations revealed the sea star-associated densovirus (SSaDV) as the most likely candidate virus associated with tissues from symptomatic asteroids. Quantification of SSaDV during transmission trials indicated that progression of SSWD paralleled increased SSaDV load. In field surveys, SSaDV loads were more abundant in symptomatic than in asymptomatic asteroids. SSaDV could be detected in plankton, sediments and in nonasteroid echinoderms, providing a possible mechanism for viral spread. SSaDV was detected in museum specimens of asteroids from 1942, suggesting that it has been present on the North American Pacific Coast for at least 72 y. SSaDV is therefore the most promising candidate disease agent responsible for asteroid mass mortality.
东北太平洋海岸至少20种海星物种的种群最近经历了海星(小行星)消瘦病(SSWD)的大规模爆发。这种疾病会导致行为变化、病变、失去膨压、肢体自切以及以快速退化(“融化”)为特征的死亡。在这里,我们提供了来自实验性挑战研究和实地观察的证据,将大规模死亡与一种浓核病毒(细小病毒科)联系起来。将来自有症状组织的病毒大小的物质(即<0.2μm)接种到无症状的海星中,始终会导致SSWD症状,而接受热灭活(即对照)病毒大小接种物的动物则保持无症状。病毒宏基因组学研究表明,海星相关浓核病毒(SSaDV)是与有症状海星组织相关的最有可能的候选病毒。在传播试验期间对SSaDV的定量分析表明,SSWD的进展与SSaDV负荷的增加平行。在实地调查中,有症状的海星中SSaDV负荷比无症状的海星中更丰富。SSaDV可以在浮游生物、沉积物和非海星棘皮动物中检测到,这为病毒传播提供了一种可能的机制。在1942年的海星博物馆标本中检测到了SSaDV,这表明它在北美太平洋海岸已经存在了至少72年。因此,SSaDV是导致海星大规模死亡的最有希望成为致病因子的候选者。