# A comparative analysis of bacterial community characterization and host–bacteria interactions between bi-macroalgal blooms caused by Ulva prolifera and Sargassum horneri

**Authors:** Yu Zang, Xiaoxue Liu, Song Xue, Lei Yin, Shiliang Fan, Xiaoxiang Miao, Mingzhu Fu, Jie Xiao, Zongling Wang

PMC · DOI: 10.3389/fmicb.2025.1728378 · Frontiers in Microbiology · 2025-12-18

## TL;DR

This study compares the bacterial communities and host-bacteria interactions in two types of macroalgal blooms in the Yellow Sea, revealing how each species recruits different microbes through unique metabolites.

## Contribution

The study identifies distinct bacterial recruitment patterns and metabolite-driven interactions in co-occurring macroalgal blooms, offering new insights into bloom dynamics.

## Key findings

- Sargassum horneri has a more diverse bacterial community than Ulva prolifera.
- U. prolifera's Verrucomicrobiae are supported by phenolic acids, while S. horneri's Gammaproteobacteria are linked to amino acids and lipids.
- Host-derived metabolites shape microbial communities, influencing macroalgal bloom persistence.

## Abstract

Macroalgal blooms have increasingly occurred in coastal regions worldwide. Since 2017, simultaneous green tides (Ulva prolifera) and golden tides (Sargassum horneri) have recurred annually in the Yellow Sea, forming a unique large-scale bi-macroalgal bloom. Interactions between macroalgae and their associated bacterial communities are recognized as key ecological drivers of algal bloom dynamics. In this study, the differences in phycosphere-associated bacterial communities and algae-derived metabolites between U. prolifera and S. horneri were explored using the 16S rRNA amplicon combined with broad-spectrum metabolomics. The results reveal that the diversity of phycospheric and epiphytic bacterial communities of S. horneri is significantly higher than that of U. prolifera. We observed distinct phycosphere bacterial recruitment between the two macroalgal species. Verrucomicrobiae were the stable core microbiota in the U. prolifera phycosphere, whereas Gammaproteobacteria and Bacteroidia represented the core members in that of S. horneri. Community assembly analyses indicate that deterministic processes predominantly shape the epiphytic bacterial communities, suggesting strong host selection effects. Metabolomic profiling further revealed that the metabolites secreted by U. prolifera, such as phenolic acids and organic acids, promote the proliferation and colonization of Verrucomicrobiae Rubritalea, which may enhance the stress tolerance of the host. In contrast, the amino acids, nucleotides, lipids, and their derivatives are key metabolites that promote the colonization of Gammaproteobacteria Vibrio and Marinomonas on the S. horneri surface, which may inhibit host growth through the production of algicidal substances. Together, these results suggest that U. prolifera and S. horneri can secrete different metabolites that recruit epiphytic microbial communities and influence macroalgae–bacteria interactions. These findings provide insights into the ecological mechanisms underlying host–bacteria interactions and their roles in the formation and persistence of macroalgal blooms.

## Linked entities

- **Species:** Ulva prolifera (taxon 3117), Sargassum horneri (taxon 74089), Gammaproteobacteria (taxon 1236), Bacteroidia (taxon 200643), Rubritalea (taxon 361050), Vibrio (taxon 662), Marinomonas (taxon 28253)

## Full-text entities

- **Diseases:** green (OMIM:614156)
- **Chemicals:** nucleotides (MESH:D009711), lipids (MESH:D008055), amino acids (MESH:D000596), organic acids (-), phenolic acids (MESH:C017616)
- **Species:** Marinomonas (genus) [taxon 28253], Sargassum horneri (species) [taxon 74089], Vibrio (genus) [taxon 662], Ulva prolifera (species) [taxon 3117], PX clade (clade) [taxon 569578]

## Full text

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## Figures

4 figures with captions in the complete paper: https://tomesphere.com/paper/PMC12756825/full.md

## References

77 references — full list in the complete paper: https://tomesphere.com/paper/PMC12756825/full.md

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Source: https://tomesphere.com/paper/PMC12756825