Division of Microbial Ecology, Centre for Microbiology and Environmental Systems Science, University of Vienna, 1030 Vienna, Austria.
Australian Institute of Marine Science, 4810 Townsville, Australia.
ISME J. 2024 Jan 8;18(1). doi: 10.1093/ismejo/wrae069.
Ammonia-oxidizing archaea and nitrite-oxidizing 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 characterize two novel nitrifying symbiont lineages, Candidatus Nitrosokoinonia and Candidatus Nitrosymbion in the marine sponge Coscinoderma matthewsi using a combination of molecular tools, in situ visualization, and physiological rate measurements. Both represent a new genus in the ammonia-oxidizing archaeal class Nitrososphaeria and the nitrite-oxidizing bacterial order Nitrospirales, respectively. Furthermore, we show that larvae of this viviparous sponge are densely colonized 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-oxidizing 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-oxidizing bacterial symbionts of the genus Ca. Nitrosymbion may reciprocally support the ammonia-oxidizers with ammonia via the utilization 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.
氨氧化古菌和亚硝酸盐氧化细菌是海洋海绵微生物组的常见成员。它们从硝化作用中获取能量来固定碳和生长——即氨的有氧氧化为亚硝酸盐,进一步氧化为硝酸盐——并被认为在海绵共生体的碳氮循环中发挥着重要作用。在这项研究中,我们使用分子工具、原位可视化和生理速率测量相结合的方法,对海洋海绵 Coscinoderma matthewsi 中的两种新型硝化共生体线系进行了表征,即候选硝化共生体 Candidatus Nitrosokoinonia 和 Candidatus Nitrosymbion。这两种共生体分别代表氨氧化古菌类 Nitrososphaeria 和亚硝酸盐氧化细菌目 Nitrospirales 的一个新属。此外,我们还表明,这种胎生海绵的幼虫被 Ca. Nitrosokoinonia 和 Ca. Nitrosymbion 的代表大量定植,表明存在垂直传播。在成体中,这两种共生体代表都位于中胶层的细胞外。比较宏基因组分析和生理数据表明,Ca. Nitrosokoinonia 属的氨氧化古菌共生体强烈依赖于内源性产生的含氮化合物(即铵、尿素、腈/氰化物和肌氨酸),而不是海绵吸收的外源性铵源。此外,Ca. Nitrosymbion 属的亚硝酸盐氧化细菌共生体可能通过利用海绵衍生的尿素和异氰酸盐来为氨氧化菌提供氨。对已发表的环境 16S rRNA 基因扩增子数据的比较分析表明,Ca. Nitrosokoinonia 和 Ca. Nitrosymbion 广泛分布,并主要与海洋海绵和珊瑚相关,这表明我们的发现具有广泛的相关性。