Abstract

In the dark ocean, the balance between the heterotrophic carbon demand and the supply of sinking carbon through the biological carbon pump remains poorly constrained. In situ tracking of the dynamics of microbial degradation processes occurring on the gravitational sinking particles is still challenging. Our particle sinking simulator system (PASS) intends to mimic as closely as possible the in situ variations in pressure and temperature experienced by gravitational sinking particles. Here, we used the PASS to simultaneously track geochemical and microbial changes that occurred during the sinking through the mesopelagic zone of laboratory-grown Emiliania huxleyi aggregates amended by a natural microbial community sampled at 105 m depth in the North Atlantic Ocean. The impact of pressure on the prokaryotic degradation of POC and dissolution of E. huxleyi-derived calcite was not marked compared to atmospheric pressure. In contrast, using global O2 consumption monitored in real-time inside the high-pressure bottles using planar optodes via a sapphire window, a reduction of respiration rate was recorded in surface-originated community assemblages under increasing pressure conditions. Moreover, using a 16S rRNA metabarcoding survey, we demonstrated a drastic difference in transcriptionally active prokaryotes associated with particles, incubated either at atmospheric pressure or under linearly increasing hydrostatic pressure conditions. The increase in hydrostatic pressure reduced both the phylogenetic diversity and the species richness. The incubation at atmospheric pressure, however, promoted an opportunistic community of “fast” degraders from the surface (Saccharospirillaceae, Hyphomonadaceae, and Pseudoalteromonadaceae), known to be associated with surface phytoplankton blooms. In contrast, the incubation under increasing pressure condition incubations revealed an increase in the particle colonizer families Flavobacteriaceae and Rhodobacteraceae, and also Colwelliaceae, which are known to be adapted to high hydrostatic pressure. Altogether, our results underline the need to perform biodegradation experiments of particles in conditions that mimic pressure and temperature encountered during their sinking along the water column to be ecologically relevant.

Highlights

  • The oceanic biological carbon pump, through a complex set of processes, removes a part of the atmospheric carbon dioxide (CO2 ), fixed by photosynthesis in the euphotic ocean, by storing it into the ocean’s interior [1,2]

  • We evaluate the hydrostatic pressure impact, as a single abiotic forcing factor, on prokaryotic diversity and activity associated with gravitational sinking particles

  • Carbohydrates were degraded in both experimental conditions since no significant differences between atmospheric pressure (ATM) and HP conditions were noticeable (Mann–Whitney pairwise test, p > 0.05)

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Summary

Introduction

The oceanic biological carbon pump, through a complex set of processes, removes a part of the atmospheric carbon dioxide (CO2 ), fixed by photosynthesis in the euphotic ocean, by storing it into the ocean’s interior [1,2]. The particle injection pumps have been proposed as an augmented BGP [3], aggregating additional transportation pathways such as water mixing process, eddy subduction, and diel or seasonal vertical migrations of fish or zooplankton. The mesopelagic or twilight zone (euphotic zone base to 1000 m depth) represents a key environment, in which gravitational sinking particles are transported and transformed [2,4], half of the flux loss being due to particle fragmentation and remineralization [5], driven by zooplankton [6,7,8] and by heterotrophic microorganisms [9,10]. It is highly relevant to estimate and understand how gravitational sinking particles are remineralized (into dissolved inorganic carbon) by heterotrophic prokaryotes through mesopelagic waters

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