Co-occurring nitrifying symbiont lineages are vertically inherited and widespread in marine sponges

Bettina Glasl, Heidi M Luter, Katarina Damjanovic, Katharina Kitzinger, Anna J Mueller, Leonie Mahler, Joan Pamela Engelberts, Laura Rix, Jay T Osvatic, Bela Hausmann, Joana Séneca, Holger Daims, Petra Pjevac, Michael Wagner
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Abstract

Ammonia-oxidising archaea and nitrite-oxidising bacteria are common members of marine sponge microbiomes. They derive energy for carbon fixation and growth from nitrification - the aerobic oxidation of ammonia to nitrite and further to nitrate - and are proposed to play essential roles in the carbon and nitrogen cycling of sponge holobionts. In this study, we characterise two novel nitrifying symbiont lineages, Candidatus Nitrosokoinonia and Candidatus Nitrosymbion in the marine sponge Coscinoderma matthewsi using a combination of molecular tools, in situ visualisation, and physiological rate measurements. Both represent a new genus in the ammonia-oxidising archaeal class Nitrososphaeria and the nitrite-oxidising bacterial order Nitrospirales, respectively. Furthermore, we show that larvae of this viviparous sponge are densely colonised by representatives of Ca. Nitrosokoinonia and Ca. Nitrosymbion indicating vertical transmission. In adults, the representatives of both symbiont genera are located extracellularly in the mesohyl. Comparative metagenome analyses and physiological data suggest that ammonia-oxidising archaeal symbionts of the genus Ca. Nitrosokoinonia strongly rely on endogenously produced nitrogenous compounds (i.e., ammonium, urea, nitriles/cyanides, and creatinine) rather than on exogenous ammonium sources taken up by the sponge. Additionally, the nitrite-oxidising bacterial symbionts of the genus Ca. Nitrosymbion may reciprocally support the ammonia-oxidisers with ammonia via the utilisation of sponge-derived urea and cyanate. Comparative analyses of published environmental 16S rRNA gene amplicon data revealed that Ca. Nitrosokoinonia and Ca. Nitrosymbion are widely distributed and predominantly associated with marine sponges and corals, suggesting a broad relevance of our findings.
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共生硝化共生菌系在海洋海绵中广泛存在并垂直遗传
氨氧化古细菌和亚硝酸盐氧化细菌是海洋海绵微生物群落的常见成员。它们从硝化作用(氨被有氧氧化成亚硝酸盐,再进一步氧化成硝酸盐)中获得固定碳和生长所需的能量,并被认为在海绵全生物体的碳氮循环中发挥着重要作用。在这项研究中,我们采用分子工具、原位可视化和生理速率测量相结合的方法,描述了海洋海绵 Coscinoderma matthewsi 中两个新的硝化共生菌系--Candidatus Nitrosokoinonia 和 Candidatus Nitrosymbion 的特征。两者分别代表了氨氧化古菌类 Nitrososphaeria 和亚硝酸盐氧化细菌目 Nitrospirales 中的一个新属。此外,我们还发现这种胎生海绵的幼虫密集地定植于 Ca.Nitrosokoinonia 和 Ca.Nitrosokoinonia和Ca.在成体中,这两个共生属的代表都位于细胞外的介壳中。元基因组比较分析和生理学数据表明,氨氧化古菌共生的 Ca.Nitrosokoinonia 的氨氧化古细菌共生体主要依靠内源产生的含氮化合物(即铵、尿素、腈/氰化物和肌酐),而不是海绵吸收的外源铵。此外,亚硝酸盐氧化细菌共生体 Ca.此外,亚硝酸盐氧化细菌共生体 Ca. Nitrosymbion 属可能会通过利用海绵衍生的尿素和氰酸盐为氨氧化酶提供氨的互惠支持。对已发表的环境 16S rRNA 基因扩增片段数据的比较分析表明,Ca.Nitrosokoinonia 和 Ca.Nitrosokoinonia 和 Ca. Nitrosymbion 分布广泛,主要与海洋海绵和珊瑚有关,这表明我们的发现具有广泛的相关性。
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