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Fueled by methane: deep-sea sponges from asphalt seeps gain their nutrition from methane-oxidizing symbionts

机译:以甲烷为燃料:沥青渗漏产生的深海海绵通过甲烷氧化共生体获得营养

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摘要

Sponges host a remarkable diversity of microbial symbionts, however, the benefit their microbes provide is rarely understood. Here, we describe two new sponge species from deep-sea asphalt seeps and show that they live in a nutritional symbiosis with methane-oxidizing (MOX) bacteria. Metagenomics and imaging analyses revealed unusually high amounts of MOX symbionts in hosts from a group previously assumed to have low microbial abundances. These symbionts belonged to the Marine Methylotrophic Group 2 clade. They are host-specific and likely vertically transmitted, based on their presence in sponge embryos and streamlined genomes, which lacked genes typical of related free-living MOX. Moreover, genes known to play a role in host–symbiont interactions, such as those that encode eukaryote-like proteins, were abundant and expressed. Methane assimilation by the symbionts was one of the most highly expressed metabolic pathways in the sponges. Molecular and stable carbon isotope patterns of lipids confirmed that methane-derived carbon was incorporated into the hosts. Our results revealed that two species of sponges, although distantly related, independently established highly specific, nutritional symbioses with two closely related methanotrophs. This convergence in symbiont acquisition underscores the strong selective advantage for these sponges in harboring MOX bacteria in the food-limited deep sea.
机译:海绵具有多种多样的微生物共生体,但是,它们的微生物所提供的益处却鲜为人知。在这里,我们描述了来自深海沥青渗流的两种新海绵物种,并表明它们生活在与甲烷氧化(MOX)细菌营养共生的环境中。荟萃基因组学和影像学分析显示,先前假设微生物丰度低的一组宿主的MOX共生体数量异常高。这些共生体属于海洋甲基营养第2族进化枝。它们是宿主特异性的,并且由于它们存在于海绵胚胎和流线型基因组中而缺乏宿主相关自由生活MOX的典型基因,因此它们可能是垂直传播的。此外,已知在宿主-共生体相互作用中起作用的基因,例如编码真核生物样蛋白的基因,已经大量表达。共生体对甲烷的吸收是海绵中表达最强的代谢途径之一。脂质的分子稳定碳同位素模式证实了甲烷衍生的碳已整合到宿主中。我们的研究结果表明,尽管有密切的联系,但两种海绵分别与两种紧密相关的甲烷营养生物独立地建立了高度特异性的营养共生体。共生体获取的这种融合强调了这些海绵在食物有限的深海中携带MOX细菌的强大选择优势。

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