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			<titleStmt><title level='a'>Prokaryotic Life in the Deep Ocean's Water Column</title></titleStmt>
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				<publisher>Annual Reviews</publisher>
				<date>01/16/2023</date>
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				<bibl> 
					<idno type="par_id">10533424</idno>
					<idno type="doi">10.1146/annurev-marine-032122-115655</idno>
					<title level='j'>Annual Review of Marine Science</title>
<idno>1941-1405</idno>
<biblScope unit="volume">15</biblScope>
<biblScope unit="issue">1</biblScope>					

					<author>Gerhard J Herndl</author><author>Barbara Bayer</author><author>Federico Baltar</author><author>Thomas Reinthaler</author>
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			<abstract><ab><![CDATA[<p>The oceanic waters below a depth of 200 m represent, in terms of volume, the largest habitat of the biosphere, harboring approximately 70% of the prokaryotic biomass in the oceanic water column. These waters are characterized by low temperature, increasing hydrostatic pressure, and decreasing organic matter supply with depth. Recent methodological advances in microbial oceanography have refined our view of the ecology of prokaryotes in the dark ocean. Here, we review the ecology of prokaryotes of the dark ocean, present data on the biomass distribution and heterotrophic and chemolithoautotrophic prokaryotic production in the major oceanic basins, and highlight the phylogenetic and functional diversity of this part of the ocean. We describe the connectivity of surface and deep-water prokaryotes and the molecular adaptations of piezophilic prokaryotes to high hydrostatic pressure. We also highlight knowledge gaps in the ecology of the dark ocean's prokaryotes and their role in the biogeochemical cycles in the largest habitat of the biosphere.</p>]]></ab></abstract>
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<div xmlns="http://www.tei-c.org/ns/1.0"><head n="1.">INTRODUCTION</head><p>The dark ocean (defined here as depths below 200 m) is characterized by low temperature, high hydrostatic pressure, and high inorganic nutrient concentrations. Comprising the mesopelagic (200-1,000 m), bathypelagic (1,000-4,000 m), abyssopelagic (4,000-6,000 m), and hadopelagic (&gt;6,000 m) zones, this ecosystem of roughly 1.3 &#215; 10 9 km 3 represents the largest habitat in the biosphere <ref type="bibr">(Bar-On et al. 2018)</ref>. Compared with the sunlit epipelagic waters, relatively little is known about dark-ocean biological processes. However, over the last two decades, research on dark-ocean microbes (the most important biological entities, particularly in the deep water column) has received considerable attention. Global ocean expeditions such as Ta ra Oceans <ref type="bibr">(Bork et al. 2015)</ref> and the Malaspina Circumnavigation Expedition <ref type="bibr">(Duarte 2015)</ref>, as well as other major deep-sea expeditions for individual research projects, have advanced our knowledge of the functioning of the dark-ocean microbiome. The previous assumption that the deep-ocean water column is characterized by low microbial abundance and metabolic activity has changed with the discovery of novel microbial metabolic pathways, refining our view of the biogeochemical cycling of organic matter by deep-sea microbes.</p><p>Here, we review and focus on the current status of knowledge of the dark ocean's prokaryotic abundance and biomass production in the meso-and bathypelagic water column, prokaryotic phylogenetic and functional diversity, vertical connectivity, and the role of hydrostatic pressure. We also highlight knowledge gaps and challenges in our understanding of the functioning of deep-sea microbes and their role in the carbon cycling of the global ocean.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="2.">PROKARYOTIC ABUNDANCE AND HETEROTROPHIC BIOMASS PRODUCTION THROUGHOUT THE WATER COLUMN</head><p>Despite the major advances in omics approaches and the resulting refined knowledge of prokaryotic metabolic capabilities, the relatively simple metrics of biomass and biomass production still provide the base to evaluate the ecological role of microbes in the aquatic environment. Since the reviews by <ref type="bibr">Ar&#237;stegui et al. (2009)</ref> and <ref type="bibr">Robinson et al. (2010)</ref>, however, advances in the classical methodologies to determine these two basic parameters have not kept pace with those based on omics approaches.</p><p>Prokaryotes in the dark ocean are fundamental for the cycling of carbon, nitrogen, and phosphorus, and it is now unequivocally clear that they are metabolically active from the surface ocean to the seafloor, remineralizing complex organic matter to inorganic nutrients and CO 2 .Inverse modeling of physical and geochemical measurements has helped us understand the cycling of elements in the global ocean; however, these models generally do not include parameterizations of the variability and magnitude of microbial heterotrophic activity that would provide a high-resolution view of biological processes in the dark ocean, which decreases the predictive power of the model outcomes. Heterotrophic activity is often used as a loose term to describe the assimilation rate of radiolabeled organic substrates by microbes, although microbial activity should encompass assessments of both production and respiration. A simple reason for this bias is the sensitivity and ease of measuring prokaryotic heterotrophic biomass production (PHP) throughout the water column, whereas the current methodology limits high-throughput measurements of respiration rates <ref type="bibr">(Robinson 2019</ref>). Yet there is a limited understanding of the global variability of prokaryotic abundance and biomass production in the water columns of major oceanic basins.</p><p>We collated a dark-ocean data set on prokaryotic abundance and heterotrophic production, including metadata spanning all major open-ocean regions. All data sources are listed in Supplemental Table <ref type="table">1</ref>. Only prokaryotic data with unambiguous metadata (cruise information, Map of stations included in the data set. Only stations off the continental shelf have been considered. The Mediterranean Sea was excluded from the analysis.</p><p>station, and longitude and latitude) were chosen for the analysis (Figure <ref type="figure">1</ref>). Fewer data are available from the stormy seasons (depending on the hemisphere) and from the Southern Hemisphere. The Indian Ocean in particular is undersampled, with essentially no data available between 0.8&#176;N and 50&#176;S. Except for the upper mesopelagic (to &#8764;500-m depth), where the data density is higher, greater depths have been sampled with roughly similar intensity (Figure <ref type="figure">2</ref>). Prokaryotic cell abundance was converted to prokaryotic biomass using a conversion factor (CF) of 10 fg C per cell, a CF typical for open-ocean prokaryotes <ref type="bibr">(Herndl et al. 2005)</ref>. We Ta bl e 1 Bacterial biomass and production in the major ocean basins Ocean Depth a Biomass b (&#181;mol C m -3 ) Production b (&#181;mol C m -3 d -1 ) CSP c (amol C cell -1</p><p>d -1 ) n d Biomass e (mmol C m -2 ) Production e (mmol C m -2 ) n d Arctic Epipelagic 335.6 &#177; 28.2 19.05 &#177; 5.34 37.5 &#177; 11.6 83 44.7 &#177; 0.2 2.09 &#177; 0.3 NA Mesopelagic 64.6 &#177; 4.3 1.55 &#177; 1.00 13.8 &#177; 9.0 43 37.0 &#177; 2.5 0.07 &#177; 0.0 7 Bathypelagic 15.7 &#177; 1.0 0.01 &#177; 0.00 0.5 &#177; 0.1 41 42.0 &#177; 0.7 0.02 &#177; 0.0 6 Atlantic Epipelagic 264.6 &#177; 4.9 16.7 &#177; 0.89 54.0 &#177; 3.1 348 69.2 &#177; 0.2 9.49 &#177; 0.2 NA Mesopelagic 87.8 &#177; 2.2 1.42 &#177; 0.11 14.8 &#177; 1.7 507 88.0 &#177; 1.9 1.83 &#177; 0.1 211 Bathypelagic 27.4 &#177; 0.7 0.22 &#177; 0.02 5.6 &#177; 0.5 869 76.0 &#177; 3.4 0.48 &#177; 0.1 95 Pacific Epipelagic 497.0 &#177; 19.3 40.93 &#177; 2.33 82.5 &#177; 6.0 532 99.1 &#177; 0.2 10.72 &#177; 0.3 NA Mesopelagic 105.7 &#177; 3.0 1.49 &#177; 0.20 11.6 &#177; 1.7 459 73.0 &#177; 3.4 0.44 &#177; 0.1 64 Bathypelagic 21.7 &#177; 0.8 0.05 &#177; 0.01 1.9 &#177; 0.1 375 74.0 &#177; 6.2 0.11 &#177; 0.0 41 Indian Epipelagic 589.2 &#177; 13.1 96.97 &#177; 3.91 121.6 &#177; 4.4 657 69.1 &#177; 0.1 6.52 &#177; 0.2 NA Mesopelagic 195.0 &#177; 10.1 9.25 &#177; 0.94 58.3 &#177; 7.3 222 112.0 &#177; 5.8 6.78 &#177; 1.0 41 Bathypelagic 41.2 &#177; 1.5 8.95 &#177; 0.89 226.4 &#177; 25.9 142 94.0 &#177; 6.2 16.28 &#177; 6.4 7 All oceans Epipelagic 476.2 &#177; 9.0 57.33 &#177; 1.98 90.0 &#177; 2.9 1,620 82.3 &#177; 0.2 10.41 &#177; 0.2 NA Mesopelagic 113.0 &#177; 2.6 2.86 &#177; 0.21 21.4 &#177; 1.7 1,231 87.0 &#177; 1.8 2.10 &#177; 0.2 323 Bathypelagic 27.0 &#177; 0.5 1.04 &#177; 0.11 26.4 &#177; 3.1 1,427 75.0 &#177; 2.8 1.10 &#177; 0.4 149 a Epipelagic, 5-200-m depth; mesopelagic, 200-1,000-m depth; or bathypelagic, 1,000-4,000-m depth. b Mean &#177; standard error of volumetric data averaged over the different depth levels. c Cell-specific bacterial production &#177; standard error. d Number of volumetric measurements. Abbreviation: NA, not applicable. e Depth-integrated values.</p><p>exclusively considered leucine incorporation (either 3 Ho r 14 C labeled) as a proxy for PHP and excluded 3 H-thymidine incorporation, a proxy for DNA synthesis and hence growth. Recently, it has been argued that 14 C-labeled leucine should be the preferred tracer for estimating PHP because leucine is prone to cleavage of methyl groups, and thus, a variable fraction of 3 H-labeled leucine will not be detected in assays; consequently, PHP might be underestimated when using 3 H-leucine <ref type="bibr">(Hill et al. 2013</ref><ref type="bibr">, Giering &amp; Evans 2022)</ref>. Most of the PHP measurements, however, were performed using 3 H-leucine. Thus, based on the above argument, there is likely some bias in the data. PHP was measured with the filter method <ref type="bibr">(Kirchman et al. 1985)</ref> and the microfuge method <ref type="bibr">(Smith &amp; Azam 1992)</ref>, with slight variations among studies. In a selected data set of the open western Atlantic, both methods correlated well over the whole water column (r 2 = 0.98, p &lt; 0.0001); however, on average, data from the filtration method are higher by 20-30% compared with parallel samples measured with the microfuge method (Supplemental Figure <ref type="figure">1</ref>).</p><p>Most studies used a leucine-to-carbon conversion of 1.5 kg C mol -1 leucine incorporated. There is considerable debate on the possible ranges of leucine CFs for PHP <ref type="bibr">(Baltar et al. 2010a</ref><ref type="bibr">, Teira et al. 2015)</ref>, varying between 0.02 and 36.4 kg C mol -1 leucine <ref type="bibr">(Giering &amp; Evans 2022)</ref>. Due to the lack of a universally applicable and consistent CF, we recalculated all data to the theoretical CFof1.5kgCmol -1 leucine <ref type="bibr">(Simon &amp; Azam 1989)</ref>. This CF might also vary with water column depth; however, experiments trying to establish CFs that take in situ pressure conditions into account have not yet been reported.</p><p>The averaged rates and stocks of prokaryotic biomass and production in the epipelagic, mesopelagic, and bathypelagic (Table <ref type="table">1</ref>) are lower by at least 50% than those published in an earlier review <ref type="bibr">(Ar&#237;stegui et al. 2009)</ref>. This is due to the vastly increased data set reported here (n = 4,300 data points), including new data from major regions of the oligotrophic subtropical gyres, the Arctic Ocean, and the Southern Ocean. We also excluded the Mediterranean Sea and</p><p>1 2 3 4 b -3 -2 -1 0 1 2 3 -3 -2 -1 0 1 2 3 log 10 (prokaryotic production) (&#956;mol C m -3 d -1 ) 13 13 1 2 3 4 a Arctic All oceans log 10 (prokaryotic biomass) (&#956;mol C m -3 ) 13 13 13 Atlantic Pacific Indian 2222 2 log 10 (depth) (m) log 10 (depth) (m)</p><p>-3 -2 -1 0 1 2 3 -3 -2 -1 0 1 2 3 -3 -2 -1 0 1 2 3</p><p>Figure <ref type="figure">3</ref> (a) Prokaryotic biomass versus depth and (b) prokaryotic production versus depth using log 10 transformed data in the Arctic Ocean, the Atlantic Ocean, the Pacific Ocean, the Indian Ocean, and all oceanic regions combined. Linear regressions on transformed data (for intercepts, slopes, and statistics, see Supplemental Table <ref type="table">3</ref>) are shown as solid gray lines. The orange squares in the far-right subpanels indicate averages of depth bins with range limits of 5, 50, 100, 200, 500, 1,000, 2,000, 3,000, 4,000, and 5,000 m (see Supplemental Ta bl e 2). The standard errors are smaller than the squares.</p><p>considered only data where both prokaryotic abundances and PHP measurements were available, yielding a congruent data set (compare Table <ref type="table">1</ref> with table 1 in <ref type="bibr">Ar&#237;stegui et al. 2009)</ref>. In all oceanic basins, prokaryotic biomass decreases exponentially between 10-and 5,000-m depth, with a biomass of 676 &#177; 18 &#181;mol C m -3 (mean &#177; standard error) at the surface and 13 &#177; 1 &#181;mol C m -3 (mean &#177; standard error) at 5,000-m depth, averaged over all ocean basins (Figure <ref type="figure">3a</ref>; Supplemental Table <ref type="table">2</ref>). The regression slopes of log-log transformed data of biomass versus depth are similar among the different ocean basins, averaging -0.73 (Figure <ref type="figure">3a</ref>; Supplemental Table <ref type="table">3</ref>). This decrease in biomass with depth is steeper than previously reported <ref type="bibr">(Ar&#237;stegui et al. 2009</ref>) and is probably due to the low quality of organic substrate required to support PHP in large parts of the open ocean's interior in the revised data set. With the exception of the Atlantic compared with the Pacific, however, significant differences in intercepts (range of 3.6-3.9; Supplemental Table <ref type="table">3</ref>) indicate that the lowest prokaryotic carbon biomass is in the Arctic Ocean and the highest is in the Indian Ocean (Figure <ref type="figure">3a</ref>).</p><p>Prokaryotic production also decreases exponentially (99.56 to 0.02 &#181;mol C m -3 d -1 )fromthe euphotic zone to the bathypelagic. Approximately 98% of prokaryotic production is attenuated from the surface to the base of the mesopelagic (Figure <ref type="figure">3b</ref>; Supplemental Table <ref type="table">2</ref>). With the exception of the Indian Ocean, all ocean basins showed similar slopes of decrease of approximately -1.57 (Supplemental Table <ref type="table">3</ref>). Most of the Indian Ocean data are from the Arabian Sea, a rather special region with restricted circulation and extensive hypoxic conditions beneath the seasonal pycnocline <ref type="bibr">(Ducklow 2000)</ref>. The Atlantic and the Pacific have similar regression intercepts and slopes, but covariance models indicate differences in the Indian Ocean and the Arctic Ocean. This might be due to a smaller variability in environmental parameters such as temperature and nutrient availability in these basins or, alternatively, to the current database focusing on specific regions in these areas.</p><p>Describing the log-log decrease in cell-specific heterotrophic activity (i.e., leucine uptake rate divided by cell abundance) with depth in the world's oceans yields a slope of -0.80 (r 2 = 0.49, p &lt; 0.0001), indicating a reduction in rates of &gt;99% from the euphotic zone to the base of the bathypelagic (data not shown). Cell-specific leucine uptake rates vary from 121 amol C cell -1 d -1 in the epipelagic to 0.5 amol C cell -1 d -1 in the bathypelagic (Table <ref type="table">1</ref>). In the Arabian Sea of the Indian Ocean, cell-specific rates are significantly higher in the meso-and bathypelagic than they are in the other oceanic regions. Excluding the Arabian Sea from the global data set decreases the overall cell-specific activity by approximately 18 amol C cell -1 d -1 . Thus, while heterotrophic prokaryotes are generally active throughout the water column, particularly in the Arctic, Atlantic, and Pacific Oceans, cell-specific production is significantly reduced in the bathypelagic and is on average between 1% and 10% of the activity in the epipelagic realm.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="3.">PATTERNS OF PROKARYOTIC BIOMASS AND HETEROTROPHIC PRODUCTION IN THE ATLANTIC AND PACIFIC</head><p>To compare the variability of prokaryotic biomass and PHP of the Atlantic and Pacific, we binned the depth-integrated data from the compiled cruises into latitudinal bands of 10&#176;(a distance of approximately 1,100 km). The large gap in data coverage of the Indian Ocean did not allow such an analysis in that ocean. In the mesopelagic and bathypelagic waters, the amount and pattern of integrated prokaryotic biomass are similar between the two oceans, with generally higher biomass in the subpolar gyres and the equatorial region (Figure <ref type="figure">4a-d</ref>). Depth-integrated PHP is generally more complex than the latitudinal biomass distribution (Figure <ref type="figure">4e-h</ref>). In the Atlantic, decreasing rates of PHP are found from the Greenland-Iceland-Norwegian Sea toward the equator, indicating the evolution of initially young water masses formed in the northern North Atlantic and decreasing bioavailability of dissolved organic matter (DOM) toward the lower latitudes (see also <ref type="bibr">Reinthaler et al. 2010)</ref>.</p><p>Increased PHP at higher latitudes is also apparent for the mesopelagic waters in the Pacific, whereas bathypelagic production shows a high latitudinal variability. The pattern in mesopelagic PHP in the Pacific has recently been interpreted to reflect the influence of sinking particulate organic carbon (POC) flux, while the pattern in PHP in the bathypelagic zone could be due to regional hydrographic features and organic carbon delivery to deep waters <ref type="bibr">(Yokokawa et al. 2013</ref><ref type="bibr">, Boeuf et al. 2019</ref><ref type="bibr">, Luo et al. 2022)</ref>. Net primary production is related to depth-integrated prokaryotic biomass or PHP in the Atlantic and Pacific data sets (Supplemental Figures <ref type="figure">2</ref> and <ref type="figure">3</ref>), supporting the finding that heterotrophic prokaryotic biomass reflects the long-term POC export  <ref type="bibr">(Hansell &amp; Ducklow 2003)</ref>, whereas PHP is indicative of the short-term input of labile and/or semilabile material <ref type="bibr">(Nagata et al. 2000)</ref>.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="4.">AUTOTROPHY VERSUS HETEROTROPHY OF PROKARYOTES</head><p>Microbial communities in the oxygenated water column of the dark ocean were initially considered to be mainly heterotrophic due to their wide capacity to incorporate amino acids into Prokaryotic production versus DIC fixation in the Atlantic (blue dots) and Pacific (orange dots). The line indicates a linear regression on log 10 transformed data. The significant regression using 701 paired data points (n) explained 45% of the variability in both measurements. Abbreviation: DIC, dissolved inorganic carbon.</p><p>biomass <ref type="bibr">(Ouverney &amp; Fuhrman 2000</ref><ref type="bibr">, Teira et al. 2006</ref>). However, evidence provided by microbial radiocarbon signatures suggested a major role of chemoautotrophy in the mesopelagic <ref type="bibr">(Hansman et al. 2009)</ref>. Archaea in particular are thought to contribute to a large fraction of dissolved inorganic carbon (DIC) fixation in the deep ocean <ref type="bibr">(Wuchter et al. 2003</ref><ref type="bibr">, Ingalls et al. 2006)</ref>. In most North Atlantic water masses, dark DIC fixation is of the same order of magnitude as PHP <ref type="bibr">(Reinthaler et al. 2010)</ref>. A compilation of available PHP and dark DIC fixation rates from the Atlantic and Pacific deep waters indicates that PHP and DIC fixation rates are positively related (Figure <ref type="figure">5</ref>).</p><p>Depth-integrated dark DIC fixation rates in North Atlantic deep waters range from 1.8 to 3.2 mmol C m -2 d -1 , corresponding to 15% to 53% of the phytoplankton export production <ref type="bibr">(Reinthaler et al. 2010)</ref>. This combined evidence has led to the conclusion that chemoautotrophic activity is substantial in the deep ocean and provides a fresh, non-sinking source of particulate organic matter (POM) to the deep ocean <ref type="bibr">(Baltar et al. 2010c</ref><ref type="bibr">, Reinthaler et al. 2010)</ref>. Additionally, recent culture experiments have shown that chemoautotrophs can release a considerable fraction (&#8764;5-15%) of their fixed DIC as dissolved organic carbon (DOC) <ref type="bibr">(Bayer et al. 2022)</ref>, which is partially composed of labile compounds that often limit heterotrophic production <ref type="bibr">(Bayer et al. 2019a)</ref>.</p><p>The main energy source fueling chemoautotrophy in the oxygenated ocean is ammonia, which is supplied via ammonification of particulate organic nitrogen (PON) <ref type="bibr">(Middelburg 2011</ref>). However, measurements of DIC fixation in the deep ocean <ref type="bibr">(Herndl et al. 2005</ref><ref type="bibr">, Reinthaler et al. 2010</ref>) are on average one order of magnitude higher than can be supported by ammonium supplied via the sinking flux of PON <ref type="bibr">(Middelburg 2011</ref><ref type="bibr">, Zhang et al. 2020</ref><ref type="bibr">, Bayer et al. 2022)</ref>. This discrepancy points toward unaccounted sources of ammonium in the deep ocean, alternative energy sources supporting chemoautotrophy, and/or a major contribution of heterotrophs to dark DIC fixation. Diel vertically migrating zooplankton and micronekton actively transport ammonium and organic nitrogen compounds to deeper water layers, averaging 8-45% of the sinking PON flux in open-ocean environments <ref type="bibr">(Steinberg et al. 2002)</ref>. In addition to ammonia, potential alternative energy sources, including reduced sulfur compounds, hydrogen, and carbon monoxide, have been proposed to make up for some of the observed discrepancies <ref type="bibr">(Reinthaler et al. 2010</ref><ref type="bibr">, Swan et al. 2011</ref><ref type="bibr">, Zhang et al. 2020</ref>) (discussed further in Section 5), but the concentrations and formation rates of these sources are most likely not sufficient in oxic deep water layers. Assimilation of inorganic carbon by heterotrophic organisms has been known for approximately 80 years <ref type="bibr">(Krebs 1941)</ref>, and its potential importance in various environments has recently been reviewed <ref type="bibr">(Braun et al. 2021)</ref>. Heterotrophic microbes fix CO 2 via a variety of carboxylation reactions as part of their central metabolism <ref type="bibr">(Erb 2011)</ref>, including fatty acid biosynthesis, leucine catabolism, purine biosynthesis, and anaplerotic pathways. The few available data on heterotrophic CO 2 fixation suggest that 1-10% of carbon in prokaryotic biomass is derived from assimilation of CO 2 <ref type="bibr">(Sorokin 1966</ref><ref type="bibr">, Roslev et al. 2004</ref>), while photoheterotrophs and methanogens encoding the serine cycle can derive up to 30% and 50%, respectively, from CO 2 <ref type="bibr">(Crowther et al. 2008</ref><ref type="bibr">, Yang et al. 2013</ref><ref type="bibr">, Palovaara et al. 2014)</ref>. Thus, in epipelagic waters, heterotrophic bacterial groups likely contribute significantly to dark DIC fixation (Alonso-S&#225;ez et al. 2010). In the dark ocean, however, heterotrophic CO 2 fixation pathways, such as anaplerosis, might be less important due to the limited availability of organic carbon.</p><p>Because of the limited input of fresh DOM into the dark ocean by convection, advection, and subduction, heterotrophic microbes rely on the flux of POM rather than on DOM <ref type="bibr">(Ar&#237;stegui et al. 2002)</ref>. However, the measured prokaryotic carbon demand in deep waters has repeatedly been reported to be significantly higher than the supply of organic carbon to the dark ocean via the sinking particle flux <ref type="bibr">(Reinthaler et al. 2006</ref><ref type="bibr">, Steinberg et al. 2008</ref><ref type="bibr">, Baltar et al. 2009</ref>). Adding the measured dark DIC fixation, representing new organic carbon in the dark ocean, to the POC flux is also insufficient to close the discrepancy between the prokaryotic heterotrophic carbon demand and POC supply <ref type="bibr">(Herndl &amp; Reinthaler 2013)</ref>. By constraining estimated dark-ocean respiration and modeling, <ref type="bibr">Giering et al. (2014)</ref> were able to reconcile the mesopelagic carbon budget at a site in the North Atlantic. However, sensitivity analysis on a published data set indicates that bacterial growth efficiencies and assumed cell carbon contents have a large effect on the magnitude of the carbon imbalance <ref type="bibr">(Burd et al. 2010</ref>) (see the sidebar titled Mismatch of Particulate Organic Carbon Flux and Prokaryotic Carbon Demand). Heterotrophic production rate measurements are significantly overestimated when measured under atmospheric pressure conditions. At 1,000-and 4,000-m depths, in situ leucine incorporation amounts to only 50-60% and 30-40%, respectively, of that measured at atmospheric pressure conditions <ref type="bibr">(Amano et al. 2022</ref>). Additionally, simulated particle flux into the ocean's interior and measured respiration under increasing hydrostatic pressure showed a substantial decline in respiration rates with increasing hydrostatic pressure <ref type="bibr">(Stief et al. 2021)</ref>. This suggests that the metabolic activity of microbes, at least on sinking particles, is greatly reduced in the deeper meso-and bathypelagic waters as compared with rates measured under atmospheric pressure conditions <ref type="bibr">(Stief et al. 2021)</ref>. Including in situ pressure effects, sinking POC contributed 60% and 100% in the Pacific and the Atlantic, respectively <ref type="bibr">(Amano et al. 2022)</ref>. Thus, accounting for the effect of hydrostatic pressure and the temporal uncoupling between supply and consumption of POC <ref type="bibr">(Uchimiya et al. 2018)</ref>, the imbalance in the deep-ocean carbon budget might be partially resolved.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="5.">PHYLOGENETIC AND FUNCTIONAL DIVERSITY</head><p>The microbial communities in the deep ocean differ from those inhabiting surface waters. A recurring feature in deep waters is the high proportion of archaea, driven mainly by the increase in the abundance of marine group I archaea, currently known as thaumarchaea, which constitute</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>MISMATCH OF PARTICULATE ORGANIC CARBON FLUX AND PROKARYOTIC CARBON DEMAND</head><p>Prokaryotic organic carbon turnover is not implemented in current ocean models despite climate change-induced temperature increases that likely have a significant impact on the metabolic activity of prokaryotes in the dark ocean. To estimate the organic carbon that is needed for prokaryotes to grow in the dark ocean, the particle flux based on sediment trap data <ref type="bibr">(Antia et al. 2001</ref><ref type="bibr">, Honjo et al. 2008</ref>) has been compared with the prokaryotic carbon demand [PCD, equal to PHP plus respiration (R)] <ref type="bibr">(Herndl &amp; Reinthaler 2013</ref><ref type="bibr">, Giering et al. 2014)</ref>. While prokaryotic production is easy to measure, respiration is generally estimated from assumed prokaryotic growth efficiency (PGE) [PGE = PHP/(PHP + R), and R = (PHP/PGE) -PHP] because obtaining precise oxygen consumption measurements as a surrogate for respiration is challenging <ref type="bibr">(Reinthaler et al. 2006</ref>). Thus, apart from missing respiration measurements, an important source of uncertainty in this simple carbon matching is the choice of CF needed to recalculate from the original measurement units (assimilation of radiolabeled substrate and oxygen) to units of carbon <ref type="bibr">(Romero-Kutzner et al. 2015</ref><ref type="bibr">, Giering &amp; Evans 2022)</ref>. Sensitivity analyses using a range of CFs together with statistical bootstrapping techniques allow the estimates to be constrained. up to 40% of total cell abundance <ref type="bibr">(Karner et al. 2001</ref><ref type="bibr">, Teira et al. 2006)</ref>. While recent genome analyses indicate that heterotrophic thaumarchaea are widespread, albeit low in abundance in the mesopelagic <ref type="bibr">(Aylward &amp; Santoro 2020</ref>), all cultivated representatives thus far are obligate chemoautotrophic ammonia oxidizers <ref type="bibr">(K&#246;nneke et al. 2005</ref><ref type="bibr">, Qin et al. 2017</ref><ref type="bibr">, Bayer et al. 2019b</ref>), carrying out the first and rate-limiting step of nitrification <ref type="bibr">(Ward 2011)</ref>. As such, their abundances and activities are tightly bound to the flux of POM from the surface waters <ref type="bibr">(Santoro et al. 2019)</ref>. In the open ocean, the highest absolute abundances of thaumarchaea are found just below the photic zone and often correlate with maximum nitrification rates <ref type="bibr">(Beman et al. 2008</ref><ref type="bibr">, Shiozaki et al. 2016)</ref>. Environmental and culture studies revealed that some thaumarchaea have the metabolic flexibility to use urea and/or cyanate for ammonia oxidation <ref type="bibr">(Bayer et al. 2016</ref><ref type="bibr">, Santoro et al. 2017</ref><ref type="bibr">, Carini et al. 2018</ref><ref type="bibr">, Kitzinger et al. 2019)</ref>, while the accessibility of other dissolved organic nitrogen sources, such as amino acids, amides, and amines, is limited and requires initial heterotrophic remineralization <ref type="bibr">(Damashek et al. 2021)</ref>. Other archaeal groups, including marine group II and III euryarchaea, make up only a small fraction of cells in the deep ocean, and most genomic evidence so far suggests heterotrophic lifestyles, with a focus on high-molecular-weight organic matter degradation (see <ref type="bibr">Santoro et al. 2019 and references therein)</ref>.</p><p>Major bacterial groups of the dark ocean include diverse Alpha-and Gammaproteobacteria, SAR406/marine group A, SAR324, SAR202, Bacteroidetes, Verrucomicrobia, Actinobacteria, and Planctomycetes <ref type="bibr">(Sunagawa et al. 2015</ref><ref type="bibr">, Salazar et al. 2016</ref><ref type="bibr">, Acinas et al. 2021)</ref>. Only a few of these groups have cultured representatives, and our knowledge of the functional diversity of these groups relies greatly on metagenomic analyses. One of the well-studied bacterial groups is the alphaproteobacterial SAR11 clade (Pelagibacterales), which constitutes approximately 20% of prokaryotic cells in the deep ocean <ref type="bibr">(Morris et al. 2002</ref><ref type="bibr">, Eiler et al. 2009)</ref>. While most subclades predominantly inhabit the surface ocean, subclade IIb is found mainly in the upper mesopelagic, and there is evidence for a piezotolerant subclade Ic present in meso-and bathypelagic waters <ref type="bibr">(Thrash et al. 2014</ref><ref type="bibr">, Giovannoni 2017)</ref>. The SAR11 clade is overall relatively conserved and evolved into niches of harvesting labile, low-molecular-weight DOM, including C1 and methylated compounds <ref type="bibr">(Giovannoni 2017 and references therein)</ref>. By contrast, members of the SAR202 cluster have evolved a different metabolic strategy to adapt to the low reactivity of deep-ocean DOM by specializing in the oxidation of relatively recalcitrant to refractory compounds (Landry</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>SUBSTRATE UPTAKE STRATEGIES OF MARINE PROKARYOTES: IS MORE REALLY MORE?</head><p>Bacteria and archaea use various strategies to consume organic carbon. In the oligotrophic ocean, prokaryotes require active uptake systems that are able to scavenge low concentrations of available DOC efficiently. Such highaffinity transporters share a common feature: the presence of substrate-binding proteins (SBPs) that trap substrate in the periplasm. ABC transporter systems represent the most abundant high-affinity transporters at all depths, and their relative contribution to metaproteomes increases from the surface to the deep ocean <ref type="bibr">(Bergauer et al. 2018)</ref>. Recent models suggest that the high affinity of ABC transport is a function of SBP abundance <ref type="bibr">(Bosdriesz et al. 2015</ref><ref type="bibr">, Norris et al. 2021)</ref>, leading to half-saturation concentrations (K M ) that are more than a thousandfold smaller than its binding protein's dissociation constant (K D ) <ref type="bibr">(Norris et al. 2021)</ref>. Consequently, prokaryotes adapted to oligotrophic conditions, such as SAR11, devote much of their energy to synthesizing SBPs <ref type="bibr">(Sowell et al. 2009</ref>) and have extraordinarily high uptake affinities <ref type="bibr">(Noell &amp; Giovannoni 2019)</ref>. However, the reliance on binding proteins to achieve high affinities comes at a high cost and precludes high growth rates <ref type="bibr">(Norris et al. 2021)</ref>, which likely represents a beneficial strategy for free-living, nonmotile prokaryotes that are confined to environments with low inputs of fresh organic matter. Hence, high abundances of transporter proteins in the deep ocean are likely the result of an adaptive response to oligotrophic conditions and do not necessarily imply high uptake rates. <ref type="bibr">et al. 2017</ref><ref type="bibr">, Liu et al. 2020</ref><ref type="bibr">, Saw et al. 2020</ref>). SAR202 bacteria are abundant members of microbial communities, increasing from an approximately 5% relative abundance in the mesopelagic to up to 30% in the bathypelagic <ref type="bibr">(Morris et al. 2004</ref><ref type="bibr">, Varela et al. 2008)</ref>, where they occupy specialized niches within deep-ocean ecosystems <ref type="bibr">(Saw et al. 2020)</ref>.</p><p>Heterotrophic production in the deep ocean is generally limited by the availability of organic carbon. In a metaproteomic study, the fraction of transporters responsible for organic matter uptake increased from approximately 23% in the euphotic layers to 39% in bathypelagic waters, suggesting an adaptation of microbial communities to the changes in the quality and quantity of organic matter in the deep ocean <ref type="bibr">(Bergauer et al. 2018)</ref>. Substrate-binding proteins of ATP-binding cassette (ABC) transporter complexes make up a major fraction of deep-ocean metaproteomes <ref type="bibr">(Bergauer et al. 2018)</ref>, potentially implying high specific affinities of these transporters by maintaining a high ratio of binding proteins to transport <ref type="bibr">(Norris et al. 2021</ref>) (see the sidebar titled Substrate Uptake Strategies of Marine Prokaryotes: Is More Really More?). Deep-sea microbes are thought to be preferentially associated with particles <ref type="bibr">(Baltar et al. 2009)</ref>, which is supported by an increase with depth in the abundances and activities of secretory enzymes catalyzing the breakdown of carbohydrates and proteins <ref type="bibr">(Baltar et al. 2010b</ref><ref type="bibr">, Zhao et al. 2020)</ref>. The higher proportion of secretory to total enzymes in the deep ocean is driven mainly by members of the Alphaproteobacteria (Rhodobacterales and Sphingomonadales) and Gammaproteobacteria (Alteromonadales and Oceanospirillales), indicating a preferential utilization of POM by these groups <ref type="bibr">(Zhao et al. 2020)</ref>.</p><p>One of the most abundant proteins found in the mesopelagic is nitrite oxidoreductase (Nxr)a metalloenzyme encoded by chemoautotrophic nitrite-oxidizing Nitrospinae bacteria <ref type="bibr">(Saito et al. 2020)</ref>. Nitrospinae are low-abundance members of deep-ocean microbial communities <ref type="bibr">(Pachiadaki et al. 2017)</ref>, and the surprisingly high abundances of Nxr have been suggested to maximize contact efficiency with scarce nitrite <ref type="bibr">(Saito et al. 2020)</ref>. Cell-specific DIC fixation measurements of Nitrospinae suggest high metabolic activity <ref type="bibr">(Pachiadaki et al. 2017</ref>), but fluxes of nitrite are unlikely to sustain the observed carbon assimilation <ref type="bibr">(Zhang et al. 2020</ref>) even when accounting for higher DIC fixation yields, as recently reported <ref type="bibr">(Bayer et al. 2022)</ref>. While direct evidence for the use of alternative energy sources by Nitrospinae in the deep ocean is lacking, nitrite oxidizers have been shown to be metabolically versatile in culture, being able to oxidize hydrogen <ref type="bibr">(Koch et al. 2014</ref>) and sulfur <ref type="bibr">(F&#252;ssel et al. 2017)</ref> or grow chemoorganoautotrophically on formate <ref type="bibr">(Koch et al. 2015</ref><ref type="bibr">, Bayer et al. 2021)</ref>.</p><p>Sulfur-driven chemolithoautotrophy might be more prevalent in the oxygenated deep ocean than was initially assumed <ref type="bibr">(Swan et al. 2011)</ref>. Detached from benthic processes, sulfur cycling is believed to be sustained mainly by lateral transport processes and particle microniches <ref type="bibr">(Callbeck et al. 2021)</ref>. Additionally, the degradation of dissolved organic sulfur compounds derived from sinking phytoplankton biomass <ref type="bibr">(Landa et al. 2019</ref>) and local secretion by diel migrating zooplankton <ref type="bibr">(Clifford et al. 2017</ref><ref type="bibr">, Tutasi &amp; Escribano 2020)</ref> generate reduced and oxidized forms of inorganic sulfur species (e.g., sulfide, thiosulfate, and sulfite) in the oxic water column <ref type="bibr">(Landa et al. 2019)</ref>. In deep waters of the eastern tropical South Pacific, taurine uptake and desulfonation genes are dominated by SAR324 bacteria and the gammaproteobacterial ARCTIC96BD-19 clade <ref type="bibr">(Landa et al. 2019 and references therein)</ref>, suggesting that sulfite generation from taurine could be further oxidized to sulfate by these groups <ref type="bibr">(Callbeck et al. 2021</ref>). SAR324 bacteria have recently been classified into multiple subclades inhabiting the entire water column <ref type="bibr">(Boeuf et al. 2021</ref><ref type="bibr">, Malfertheiner et al. 2022</ref>), but the highest abundances are found in meso-and bathypelagic waters <ref type="bibr">(Ghiglione et al. 2012</ref><ref type="bibr">, Malfertheiner et al. 2022</ref>). SAR324 bacteria are metabolically diverse, and subclades present in the deep ocean share genomic features of a mixotrophic lifestyle, including sulfur-based chemolithoautotrophy and C1 compound metabolism <ref type="bibr">(Swan et al. 2011</ref><ref type="bibr">, Sheik et al. 2013</ref><ref type="bibr">, Boeuf et al. 2021)</ref>.</p><p>Trace gases such as carbon monoxide (CO) and hydrogen (H 2 ) have been suggested as potential alternative energy sources fueling dark DIC fixation <ref type="bibr">(Anantharaman et al. 2013</ref><ref type="bibr">, Zhang et al. 2020)</ref>, and genes for trace gas oxidation are widespread and abundant in deep waters <ref type="bibr">(Acinas et al. 2021</ref><ref type="bibr">, Lappan et al. 2022)</ref>. The consumption of CO and H 2 in surface waters is significant <ref type="bibr">(Xie et al. 2005</ref><ref type="bibr">, Lappan et al. 2022</ref>) and coincides with their production via photochemical oxidation and cyanobacterial N 2 fixation, respectively <ref type="bibr">(Moore et al. 2009)</ref>. High concentrations of H 2 are also found at hydrothermal vent sites <ref type="bibr">(McCollom 2008)</ref> or during fermentation in anoxic environments <ref type="bibr">(Kessler et al. 2019)</ref>. Accordingly, high abundances of hydrogenases are found in hydrothermal plumes <ref type="bibr">(Anantharaman et al. 2013</ref>) and on particles that might provide anoxic microniches <ref type="bibr">(Acinas et al. 2021</ref>). However, CO and H 2 are probably not readily available to most free-living deep-ocean prokaryotes.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="6.">PARTICLES AS VEHICLE FOR MICROBES AND CONNECTIVITY OF PROKARYOTIC COMMUNITIES</head><p>There are two fractions of detrital POM in the oceanic water column, which are differentiated by their size and specific density: neutrally buoyant suspended particles and sinking particles <ref type="bibr">(Bochdansky et al. 2010</ref><ref type="bibr">, Herndl &amp; Reinthaler 2013)</ref>. Generally, most of the detrital POM in the deep ocean consists of suspended particles <ref type="bibr">(Kepkay 2000</ref><ref type="bibr">, Verdugo et al. 2004</ref>). The depth distributions of the suspended and sinking detrital POM in the open ocean differ. The concentration of suspended POC remains relatively constant with depth <ref type="bibr">(Baltar et al. 2010c</ref>), whereas the concentration of sinking POC exponentially decreases with depth <ref type="bibr">(Martin et al. 1987</ref><ref type="bibr">, Buesseler et al. 2007)</ref>. While the origin of sinking POM is associated with phytoplankton blooms in euphotic layers, the source of suspended POM remains unclear <ref type="bibr">(Herndl &amp; Reinthaler 2013)</ref>. Suspended POM could originate either from remnants of sinking particles fragmented by deep-ocean organisms or from autochthonous production by deep-water prokaryotes via chemolithoautotrophic activity <ref type="bibr">(Baltar et al. 2010c)</ref>.</p><p>The ubiquitous occurrence of different types of detrital particles in the oceanic water column plays a key role in the distribution and activities of marine microbes. Investigations performed in deep and surface waters at specific sites <ref type="bibr">(Ghiglione et al. 2007</ref><ref type="bibr">, Eloe et al. 2011b</ref><ref type="bibr">, Crespo et al. 2013</ref><ref type="bibr">, Duret et al. 2019</ref><ref type="bibr">, Mestre et al. 2020</ref>) are in agreement with a global bathypelagic ocean analysis from the Malaspina Circumnavigation Expedition <ref type="bibr">(Salazar et al. 2015)</ref>. This analysis revealed a niche partitioning and differences in alpha and beta diversity between free-living and particleassociated microbial (nominal size cutoff 0.8 &#181;m) communities at a global scale. The study's authors used the particle-association niche index <ref type="bibr">(Stegen et al. 2012)</ref> to distinguish the preferences of microbes for a particle-associated or free-living lifestyle <ref type="bibr">(Salazar et al. 2015)</ref>. Applying this index to bathypelagic waters revealed that archaea (both euryarchaea and thaumarchaea) and the bacterial groups SAR86, SAR324, SAR406, and SAR202 exhibited a preference for a free-living lifestyle; Bacteroidetes, Firmicutes, Planctomycetes, Deltaproteobacteria clade OM27, and Desulfuromonadales were associated with particles <ref type="bibr">(Salazar et al. 2015)</ref>. <ref type="bibr">Acinas et al. (2021)</ref> showed that these major differences in the community composition of deep-ocean particle-attached and free-living communities also translate into pronounced differences in functional diversity (Figure <ref type="figure">6</ref>). These authors found that nitrification and CO oxidation genes were associated mostly with free-living assemblages, and H 2 oxidation genes were essentially linked to the particle-attached microbes. These pronounced differences in functional and phylogenetic diversity between free-living and particle-attached microbes provide even more evidence of the heterogeneous nature of the dark ocean and are a further indicator of the contrasting ecological niches that the deep ocean's particleattached and free-living microbes occupy (Figure <ref type="figure">6</ref>).</p><p>Contrasting factors are apparently controlling the free-living and particle-attached microbes in the deep ocean. Global circulation and water mass age are the parameters that more strongly affect the particle-attached microbes, whereas temperature and depth control the composition of free-living communities <ref type="bibr">(Salazar et al. 2016)</ref>. Surprisingly, the deep-ocean particle-attached microbiome but not the free-living microbiome showed indications of dispersal limitation and, consequently, basin specificity <ref type="bibr">(Salazar et al. 2016)</ref>. This is consistent with the notion that a significant portion of the deep-ocean particles colonized by microbes is not sinking POM but suspended particles <ref type="bibr">(Baltar et al. 2009</ref><ref type="bibr">(Baltar et al. , 2010c;;</ref><ref type="bibr">Herndl &amp; Reinthaler 2013)</ref>. Deep-ocean microbial respiration has been associated with suspended particles <ref type="bibr">(Baltar et al. 2009</ref><ref type="bibr">, Bochdansky et al. 2010)</ref>. A high proportion of dissolved versus total extracellular enzymatic activities has been reported in the deep sea measured with substrate analogs <ref type="bibr">(Baltar 2018;</ref><ref type="bibr">Baltar et al. 2010a</ref><ref type="bibr">Baltar et al. , 2013))</ref>, which, based on the foraging theory (i.e., the theory that natural selection favors strategies of organisms to maximize net energy intake per unit time spent foraging; MacArthur &amp; Pianka 1966) strongly suggests a preferential particle-attached lifestyle of dark-ocean microorganisms <ref type="bibr">(Ar&#237;stegui et al. 2009;</ref><ref type="bibr">Baltar et al. 2009</ref><ref type="bibr">Baltar et al. , 2010b))</ref>. A recent global survey on peptidases and carbohydrate-active enzymes-the two central enzyme groups targeting the two most abundant macromolecules in the ocean-revealed an increasing proportion of genes encoding secreted (i.e., dissolved) enzymes with depth <ref type="bibr">(Zhao et al. 2020)</ref>.</p><p>Deep-sea microbial communities are to a certain extent connected to surface assemblages <ref type="bibr">(Cram et al. 2015a,b;</ref><ref type="bibr">Parada &amp; Fuhrman 2017)</ref>. <ref type="bibr">Cram et al. (2015b)</ref> used a microbial association network to study the connection between community dynamics and environmental parameters within and between depth layers over a seasonal cycle. They found lagged and concurrent shifts in community composition between depths, indicating that deep-ocean free-living assemblages are linked to environmental conditions and/or communities in overlying waters. This connection between communities from different depth layers is probably due to migrating organisms transporting nutrients across otherwise stratified waters <ref type="bibr">(Maas et al. 2020</ref>) and/or sinking particles transporting cells originating from overlying waters <ref type="bibr">(Mestre et al. 2018</ref>). Thus, Illustration of free-living and particle-associated lifestyles of prokaryotes in the deep ocean. The different shapes and colors of the prokaryotic cells represent their phylogenetic and functional diversity. Prokaryotic abundances and distances between individual cells are not to scale but rather illustrate a hot spot of prokaryotic abundance and activity in the deep ocean. The abundances of particle-attached prokaryotes are on average three orders of magnitude higher than those of free-living prokaryotes. Assuming an even distribution of cells, the distance between free-living prokaryotes is 1,000 times larger than their size (equivalent to 1-cm-long cells that are 10 m apart from one another in every direction). Abbreviations: DOM, dissolved organic matter; POM, particulate organic matter.</p><p>the sunlit community composition and environmental conditions ultimately impact the microbial community on deep-water particles (Ruiz-Gonz&#225;lez et al. 2020), which is consistent with the observed influence of phytoplankton community composition and grazing on the nutritional properties of sinking particles <ref type="bibr">(Boyd &amp; Newton 1995</ref><ref type="bibr">, Guidi et al. 2016</ref><ref type="bibr">, Bach et al. 2019)</ref>. Consistently, the majority of the particle-associated prokaryotes detected in the bathypelagic are also found in epipelagic waters <ref type="bibr">(Mestre et al. 2018)</ref>.</p><p>Due to the fluctuating nature of the productivity of sunlit surface waters, it is expected that the connection between surface and deep-water prokaryotes via sinking particles varies seasonally <ref type="bibr">(Poff et al. 2021)</ref>. Moreover, the vertical structure of the water column also changes seasonally, which might also influence the connection between euphotic and deep-ocean microbial communities. A recent time-series study over a seasonal cycle of the microbial composition of surface and mesopelagic waters showed that the link between surface and deep-ocean microbial communities is not just unidirectional (via sinking of particles) <ref type="bibr">(Wenley et al. 2021)</ref>. Based on their results, the study's authors concluded that the mechanisms connecting surface and mesopelagic microbial communities change seasonally, that is, via sinking particles during the productive season (spring and summer) and via deep mixing that brings deep-water taxa into the sunlit waters during winter overturning <ref type="bibr">(Wenley et al. 2021)</ref>. The influence of this mechanism is restricted to the depth of winter convective mixing.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head n="7.">ADAPTATIONS TO HIGH HYDROSTATIC PRESSURE AND LOW TEMPERATURE BY DEEP-SEA PROKARYOTES</head><p>The extent to which deep-sea prokaryotic communities are adapted to the hydrostatic pressure conditions remains enigmatic. While some studies report elevated activity of bathypelagic heterotrophic prokaryotic communities under in situ pressure conditions as compared with corresponding measurements under decompressed conditions, other studies report opposite findings (summarized in <ref type="bibr">Tamburini et al. 2013)</ref>. Since the pioneering work in deep-sea microbiology reviewed by <ref type="bibr">Jannasch &amp; Taylor (1984)</ref>, it has been well known that there are piezophilic bacteria in the deep ocean <ref type="bibr">(Lauro &amp; Bartlett 2008)</ref>. However, the fraction of piezophilic prokaryotes within the total abundance of deep-sea prokaryotes remains unknown.</p><p>On a community level, deep-sea prokaryotes are characterized by having larger genomes than their euphotic counterparts, which is indicative of a more opportunistic lifestyle prevailing in deep waters <ref type="bibr">(DeLong et al. 2006</ref>). While only one piezophilic archaeon (Pyrococcus yayanosii) has been isolated thus far <ref type="bibr">( Jun et al. 2011)</ref>, a considerable number of piezophilic bacteria have been isolated and their genomes characterized <ref type="bibr">(Eloe et al. 2011a</ref><ref type="bibr">, Jun et al. 2011</ref><ref type="bibr">, Kusube et al. 2017)</ref>, allowing the identification of some specific features of piezophilic bacteria. The abovementioned archaeon Pyrococcus yayanosii is a thermopiezophilic representative, but most of the deep-sea piezophilic prokaryotes are psychropiezophiles (i.e., adapted to high hydrostatic pressure and low temperature). Most of the psychropiezophilic isolates belong to the Gammaproteobacteria, with representatives of Colwellia, Shewanella, Photobacterium, Moritella,andPsychromonas <ref type="bibr">(Eloe et al. 2011a</ref><ref type="bibr">, Jebbar et al. 2015</ref><ref type="bibr">, Nogi 2017)</ref>. Surprisingly, a large number of these piezophilic strains have been isolated from deep-sea amphipods <ref type="bibr">(Kusube et al. 2017)</ref>.</p><p>Comparison of genes and proteins of piezophilic versus piezosensitive Colwellia isolates revealed several features specific to the piezophilic lifestyle <ref type="bibr">(Peoples et al. 2020)</ref>. Evaluating the isoelectric point distributions of the Colwellia proteomes revealed a higher number of basic proteins in piezophilic compared with piezosensitive strains. Amino acid abundances in conserved, orthologous proteins in piezophilic Colwellia strains were enriched in tryptophan, tyrosine, leucine, phenylalanine, histidine, and methionine compared with those of piezosensitive strains <ref type="bibr">(Peoples et al. 2020)</ref>. The amino acid species enriched in piezosensitive Colwellia strains were glutamic acid, aspartic acid, asparagine, and serine (see the sidebar titled Hydrostatic Pressure and Low Temperature).</p><p>Comparing the relative abundances of clusters of orthologous genes, Peoples et al. (2020) found a higher percentage of genes for replication, recombination, and repair; cell wall and membrane biogenesis; cell motility; extracellular structures and translation; and ribosomal structures in piezophilic Colwellia strains than in piezosensitive Colwellia strains. Piezophilic and psychrophilic strains have a higher content of polyunsaturated fatty acids to increase membrane fluidity under high hydrostatic pressure and low temperature <ref type="bibr">(Peoples et al. 2020)</ref>. Another apparent adaptation to high hydrostatic pressure is the high abundance of glycosyltransferases, enzymes promoting extracellular polysaccharide synthesis <ref type="bibr">(Peoples et al. 2020)</ref>.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>HYDROSTATIC PRESSURE AND LOW TEMPERATURE</head><p>The mesopelagic and (particularly) bathypelagic global ocean is characterized by low temperatures, ranging from 0&#176;C to 4&#176;C. Only the deep waters of the Mediterranean Sea, the Red Sea, and the Sulu Sea have higher deep-water temperatures (up to 20&#176;C). Hence, piezophilic prokaryotes should typically also be adapted to low temperatures. The commonly accepted definition of piezophily is that the maximum growth rate of piezophiles occurs at pressures above the atmospheric pressure of 0.1 MPa. Typically, however, the piezosphere is considered to be depths below 1,000 m, corresponding to 10 MPa <ref type="bibr">(Yayanos 1986)</ref>. Consequently, piezophiles exhibit maximum growth rates at &gt;10 MPa <ref type="bibr">( Jannasch &amp; Taylor 1984)</ref>. As stated recently, only 86 prokaryotic isolates with a growth optimum at &gt;0.1 MPa are currently available <ref type="bibr">(Scoma 2021)</ref>.</p><p>In a general sense, hydrostatic pressure influences the intermolecular distances and thereby affects the conformation of polynucleotides (DNA and RNA), lipid bilayers, and the tertiary structure of proteins <ref type="bibr">(Oger &amp; Jebbar 2010</ref><ref type="bibr">, Scoma 2021</ref>). Thus, it seems logical that piezophilic prokaryotes should have a selective advantage over nonpiezophilic prokaryotes in the deep ocean. In a meta-analysis, Scoma (2021) took into account the interactive effect of hydrostatic pressure and temperature, determining the growth optimum based on the initial work of <ref type="bibr">Yayanos (1986)</ref> to define piezophiles. Scoma (2021) differentiated three functional groups based on temperature: piezopsychrophiles, piezomesophiles, and piezothermophiles. A competitive advantage of piezophiles over piezosensitives is predicted to begin at 10 MPa and to exist consistently irrespective of temperature at hydrostatic pressures above 20 MPa. Hyper-piezopsychrophiles are specific to hadal trenches, and their competitive advantage over piezopsychrophiles begins at a hydrostatic pressure above 50 MPa <ref type="bibr">(Scoma 2021)</ref>.</p><p>Based on the results described above, it appears that a piezophilic lifestyle of heterotrophic prokaryotes requires many changes throughout the cell. Many piezophile enriched genes are located near areas of genomic variability and could be shared among piezophiles via horizontal gene transfer.</p></div>
<div xmlns="http://www.tei-c.org/ns/1.0"><head>FUTURE ISSUES</head><p>1. Dark-ocean prokaryotic heterotrophic production has been routinely measured; however, the leucine-to-carbon conversion factor required to estimate production rates is rarely determined in the deep ocean. The few data available on leucine-to-carbon conversion factors for the deep-ocean prokaryotes are highly variable.</p><p>2. While there is a fairly large data set available on heterotrophic production, there is a severe lack of measurements of respiration, which typically contributes much more to the heterotrophic prokaryotic carbon demand than biomass production. Thus, there is a major uncertainty in the estimates of the prokaryotic heterotrophic carbon demand in the dark ocean. Metabolic rate measurements on deep-sea microbes should be performed under in situ pressure conditions. The fraction of piezophilic and piezotolerant microbes in the deep sea should be determined, since we do not know how large the fraction of piezophilic and piezotolerant microbes actually is.</p><p>3. New sampling tools and techniques are required to selectively sample detrital particles (marine snow) in the meso-and bathypelagic waters, as these particles are largely very fragile but densely populated by prokaryotes. Metabolic rate measurements on these</p></div><note xmlns="http://www.tei-c.org/ns/1.0" place="foot" xml:id="foot_0"><p>www.annualreviews.org &#8226; Prokaryotic Life in the Deep Ocean</p></note>
			<note xmlns="http://www.tei-c.org/ns/1.0" place="foot" xml:id="foot_1"><p>Annu. Rev. Mar. Sci. 2023.15:461-483. Downloaded from www.annualreviews.org Access provided by 2600:4040:25f2:2300:309e:74dc:21f2:53ad on 08/18/23. See copyright for approved use.</p></note>
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