| Literature DB >> 24277737 |
Hiroshi Mori1, Fumito Maruyama, Hiromi Kato, Atsushi Toyoda, Ayumi Dozono, Yoshiyuki Ohtsubo, Yuji Nagata, Asao Fujiyama, Masataka Tsuda, Ken Kurokawa.
Abstract
The deep sequencing of 16S rRNA genes amplified by universal primers has revolutionized our understanding of microbial communities by allowing the characterization of the diversity of the uncultured majority. However, some universal primers also amplify eukaryotic rRNA genes, leading to a decrease in the efficiency of sequencing of prokaryotic 16S rRNA genes with possible mischaracterization of the diversity in the microbial community. In this study, we compared 16S rRNA gene sequences from genome-sequenced strains and identified candidates for non-degenerate universal primers that could be used for the amplification of prokaryotic 16S rRNA genes. The 50 identified candidates were investigated to calculate their coverage for prokaryotic and eukaryotic rRNA genes, including those from uncultured taxa and eukaryotic organelles, and a novel universal primer set, 342F-806R, covering many prokaryotic, but not eukaryotic, rRNA genes was identified. This primer set was validated by the amplification of 16S rRNA genes from a soil metagenomic sample and subsequent pyrosequencing using the Roche 454 platform. The same sample was also used for pyrosequencing of the amplicons by employing a commonly used primer set, 338F-533R, and for shotgun metagenomic sequencing using the Illumina platform. Our comparison of the taxonomic compositions inferred by the three sequencing experiments indicated that the non-degenerate 342F-806R primer set can characterize the taxonomic composition of the microbial community without substantial bias, and is highly expected to be applicable to the analysis of a wide variety of microbial communities.Entities:
Keywords: 16S rRNA; microbial community; non-degenerate primer; primer design
Mesh:
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Year: 2013 PMID: 24277737 PMCID: PMC3989492 DOI: 10.1093/dnares/dst052
Source DB: PubMed Journal: DNA Res ISSN: 1340-2838 Impact factor: 4.458
Figure 1.A partial plot of the consensus sequence in each window and its coverage rate for each phylum from 531 16S rRNA genes of genome-sequenced strains. The number of species in each phylum is indicated in parentheses. The start position of each window is represented according to the corresponding position in the 16S rRNA gene from Escherichia coli. The consensus sequence in each window is represented at the bottom of the figure. Each line indicate the coverage rate for the consensus sequence of each phylum by using the colours of dots: black <50%, blue <80%, green <90%, yellow <100%, and red = 100%. The bar graph at the top of the figure indicates the sequence variability of each window that is depicted by (i) calculating the relative entropy of four nucleotides and the gap (−) at each site[38] and (ii) summing up the relative entropy of each site in the window.
Figure 2.The coverage for our universal primer set (red) and the 17 other universal primers in each of the bacterial and archaeal phyla rRNA genes, and the chloroplastic, mitochondrial, and eukaryotic rRNA genes. Each column indicates the coverage for a candidate sequence from each of the bacterial and archaeal phyla rRNA genes, and the chloroplastic, mitochondrial, and eukaryotic rRNA genes by colour intensity: blue = low coverage, and pale orange = high coverage. See Supplementary Table S1 for each sequence. The number of genera is provided in parentheses.
Figure 3.Phylum-level taxonomic compositions of prokaryotes in the soil metagenome on the basis of the 338F-533R and 342F-806R amplicon pyrosequencing and the 16S rRNA gene fragments from Illumina metagenomic sequencing. The top 18 abundant phyla from the results of Illumina metagenomic sequencing are listed.
Figure 4.Comparison of three experiments for rank abundances of phyla. Large circles indicate the rank abundances of each phylum in the three experiments, starting at the rank abundance 1, followed by 6, 11, 16, 21, and 26. Phyla are listed in a clockwise direction according to the rank abundance in the Illumina experiment.