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通过金藻鞭毛虫的比较基因组学揭示营养驱动的基因组进化

Nutrient-driven genome evolution revealed by comparative genomics of chrysomonad flagellates.

作者信息

Majda Stephan, Beisser Daniela, Boenigk Jens

机构信息

Department of Biodiversity, University of Duisburg-Essen, Essen, Germany.

出版信息

Commun Biol. 2021 Mar 12;4(1):328. doi: 10.1038/s42003-021-01781-3.

Abstract

Phototrophic eukaryotes have evolved mainly by the primary or secondary uptake of photosynthetic organisms. A return to heterotrophy occurred multiple times in various protistan groups such as Chrysophyceae, despite the expected advantage of autotrophy. It is assumed that the evolutionary shift to mixotrophy and further to heterotrophy is triggered by a differential importance of nutrient and carbon limitation. We sequenced the genomes of 16 chrysophyte strains and compared them in terms of size, function, and sequence characteristics in relation to photo-, mixo- and heterotrophic nutrition. All strains were sequenced with Illumina and partly with PacBio. Heterotrophic taxa have reduced genomes and a higher GC content of up to 59% as compared to phototrophic taxa. Heterotrophs have a large pan genome, but a small core genome, indicating a differential specialization of the distinct lineages. The pan genome of mixotrophs and heterotrophs taken together but not the pan genome of the mixotrophs alone covers the complete functionality of the phototrophic strains indicating a random reduction of genes. The observed ploidy ranges from di- to tetraploidy and was found to be independent of taxonomy or trophic mode. Our results substantiate an evolution driven by nutrient and carbon limitation.

摘要

光合真核生物主要通过对光合生物的一次或二次摄取而进化。尽管自养具有预期优势,但在诸如金藻纲等各种原生生物类群中,多次出现了向异养的转变。据推测,向混合营养进而向异养的进化转变是由营养和碳限制的不同重要性引发的。我们对16个金藻菌株的基因组进行了测序,并就其与光合、混合营养和异养营养相关的大小、功能和序列特征进行了比较。所有菌株都使用Illumina测序,部分还使用了PacBio测序。与光合类群相比,异养类群的基因组有所减少,GC含量高达59%。异养生物具有一个大的泛基因组,但核心基因组较小,这表明不同谱系存在差异特化。混合营养生物和异养生物的泛基因组合在一起,但仅混合营养生物的泛基因组并不涵盖光合菌株的完整功能,这表明基因存在随机减少。观察到的倍性范围从二倍体到四倍体,且发现其与分类学或营养模式无关。我们的结果证实了由营养和碳限制驱动的进化。

https://cdn.ncbi.nlm.nih.gov/pmc/blobs/2c15/7954800/bbcdbc17fe23/42003_2021_1781_Fig1_HTML.jpg

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