scholarly journals Microbial Loop Dynamics in Antarctic Sea-Ice

2021 ◽  
Author(s):  
◽  
Andrew Robert Martin

<p>Sea-ice is a predominant feature of polar oceans and exerts a unique influence on marine ecosystems. The annual circumpolar expansion of sea-ice around Antarctica provides a stable platform for the in situ colonisation and growth of a diverse assemblage of microbes that are integral to the energy base of the Southern Ocean. An active microbial loop has been proposed to operate within the ice matrix connecting bacteria, microalgae and protozoa, but validating this metabolic pathway has historically relied on bulk correlations of chlorophyll a (a surrogate for microalgal biomass) and estimates of bacterial production or abundance. I investigate the microbial loop using a range of physiological, genetic, and ecological techniques to determine whether the photosynthate exuded by phototrophic microalgae serves as a growth substrate for heterotrophic bacteria. This link is examined at a range of spatial (in vitro and in situ experiments) and temporal (8 hours to 18 days) scales by manipulating the supply of algal-derived photosynthate and documenting the subsequent change in bacterial metabolic activity, cell abundance and community composition. Single-cell analysis of both bacterial membrane integrity and intracellular activity revealed that sea ice is among the most productive microbial habitats. In short-term in vitro experiments, increased availability of dissolved organic matter (DOM) was shown to elicit a rapid metabolic response in sea ice bacteria, however single-activity was significantly reduced in treatments where photosynthate was restricted by either removing the majority of algal cells or inhibiting photosynthesis with 3-(3,4-dichlorophenyl)-1,1-dimethylurea (DCMU). To verify this metabolic response, microcosm simulations were conducted over a period of 9 days with microbes derived from two regions of the ice (bottom layer and high-salinity surface region) with presumed differences in the concentration of DOM. Metabolic activity was relatively low in bacteria derived from the high-saline region of the ice and in cultures spiked with DCMU, photosynthate limitation restricted bacterial growth and significantly influenced community structure. In contrast, the bottom of the ice is characterised by a high concentration of DOM and bacterial metabolic activity was shown to be higher and DCMU was less influential with respect to changes in bacterial abundance or community composition. To examine in situ microbial dynamics, a series of cores were extracted from Antarctic sea-ice and reinserted into the ice matrix upside down to expose resident microbial assemblages to a significantly different light, temperature and salinity regime. Limited assimilation of algal-derived DOM by bacteria in ice cores that were flipped illustrated a malfunction in the microbial loop after a period of 18 days. Bacteria originally at the bottom of the sea ice appeared to be temperature-limited, while a lack of growth in cells originally at the top of the ice profile was attributed to a community dominated by slow-growing psychrophilic species. A stronger physiological response to disturbance was elicited by microalgae and significant growth was contrasted with severe bleaching and cell death. This reciprocal transplant is the first of its kind to examine the in situ sea ice community and illustrats that although microbial assemblages are similar with respect to trophic dynamics, they are also attuned to distinct regions within the ice. The bacterial assimilation of algal-derived DOM is of fundamental importance to the microbial loop and by confirming that photosynthate is a major stimulus for bacterial growth, these results provide a new and unique insight into microbial dynamics in Antarctic sea-ice.</p>

2021 ◽  
Author(s):  
◽  
Andrew Robert Martin

<p>Sea-ice is a predominant feature of polar oceans and exerts a unique influence on marine ecosystems. The annual circumpolar expansion of sea-ice around Antarctica provides a stable platform for the in situ colonisation and growth of a diverse assemblage of microbes that are integral to the energy base of the Southern Ocean. An active microbial loop has been proposed to operate within the ice matrix connecting bacteria, microalgae and protozoa, but validating this metabolic pathway has historically relied on bulk correlations of chlorophyll a (a surrogate for microalgal biomass) and estimates of bacterial production or abundance. I investigate the microbial loop using a range of physiological, genetic, and ecological techniques to determine whether the photosynthate exuded by phototrophic microalgae serves as a growth substrate for heterotrophic bacteria. This link is examined at a range of spatial (in vitro and in situ experiments) and temporal (8 hours to 18 days) scales by manipulating the supply of algal-derived photosynthate and documenting the subsequent change in bacterial metabolic activity, cell abundance and community composition. Single-cell analysis of both bacterial membrane integrity and intracellular activity revealed that sea ice is among the most productive microbial habitats. In short-term in vitro experiments, increased availability of dissolved organic matter (DOM) was shown to elicit a rapid metabolic response in sea ice bacteria, however single-activity was significantly reduced in treatments where photosynthate was restricted by either removing the majority of algal cells or inhibiting photosynthesis with 3-(3,4-dichlorophenyl)-1,1-dimethylurea (DCMU). To verify this metabolic response, microcosm simulations were conducted over a period of 9 days with microbes derived from two regions of the ice (bottom layer and high-salinity surface region) with presumed differences in the concentration of DOM. Metabolic activity was relatively low in bacteria derived from the high-saline region of the ice and in cultures spiked with DCMU, photosynthate limitation restricted bacterial growth and significantly influenced community structure. In contrast, the bottom of the ice is characterised by a high concentration of DOM and bacterial metabolic activity was shown to be higher and DCMU was less influential with respect to changes in bacterial abundance or community composition. To examine in situ microbial dynamics, a series of cores were extracted from Antarctic sea-ice and reinserted into the ice matrix upside down to expose resident microbial assemblages to a significantly different light, temperature and salinity regime. Limited assimilation of algal-derived DOM by bacteria in ice cores that were flipped illustrated a malfunction in the microbial loop after a period of 18 days. Bacteria originally at the bottom of the sea ice appeared to be temperature-limited, while a lack of growth in cells originally at the top of the ice profile was attributed to a community dominated by slow-growing psychrophilic species. A stronger physiological response to disturbance was elicited by microalgae and significant growth was contrasted with severe bleaching and cell death. This reciprocal transplant is the first of its kind to examine the in situ sea ice community and illustrats that although microbial assemblages are similar with respect to trophic dynamics, they are also attuned to distinct regions within the ice. The bacterial assimilation of algal-derived DOM is of fundamental importance to the microbial loop and by confirming that photosynthate is a major stimulus for bacterial growth, these results provide a new and unique insight into microbial dynamics in Antarctic sea-ice.</p>


2012 ◽  
Vol 24 (6) ◽  
pp. 547-553 ◽  
Author(s):  
Andrew Martin ◽  
Andrew McMinn ◽  
Simon K. Davy ◽  
Marti J. Anderson ◽  
Hilary C. Miller ◽  
...  

AbstractSea ice microalgae actively contribute to the pool of dissolved organic matter (DOM) available for bacterial metabolism, but this link has historically relied on bulk correlations between chlorophylla(a surrogate for algal biomass) and bacterial abundance. We incubated microbes from both the bottom (congelation layer) and surface brine region of Antarctic fast ice for nine days. Algal-derived DOM was manipulated by varying the duration of irradiance, restricting photosynthesis with 3-(3,4-dichlorophenyl)-1,1-dimethylurea (DCMU) or incubating in the dark. The bacterial response to changes in DOM availability was examined by performing cell counts, quantifying bacterial metabolic activity and examining community composition with denaturing gradient gel electrophoresis. The percentage of metabolically active bacteria was relatively low in the surface brine microcosm (10–20% of the bacterial community), the treatment with DCMU indirectly restricted bacterial growth and there was some evidence for changes in community structure. Metabolic activity was higher (35–69%) in the bottom ice microcosm, and while there was no variation in community structure, bacterial growth was restricted in the treatment with DCMU compared to the light/dark treatment. These results are considered preliminary, but provide a useful illustration of sea ice microbial dynamics beyond the use of ‘snapshot’ biomass correlations.


2008 ◽  
Author(s):  
A Martin ◽  
JA Hall ◽  
R O’Toole ◽  
SK Davy ◽  
KG Ryan

2009 ◽  
Vol 75 (23) ◽  
pp. 7570-7573 ◽  
Author(s):  
Andrew Martin ◽  
Julie Hall ◽  
Ken Ryan

ABSTRACT Experiments simulating the sea ice cycle were conducted by exposing microbes from Antarctic fast ice to saline and irradiance regimens associated with the freeze-thaw process. In contrast to hypersaline conditions (ice formation), the simulated release of bacteria into hyposaline seawater combined with rapid exposure to increased UV-B radiation significantly reduced metabolic activity.


2011 ◽  
Vol 23 (4) ◽  
pp. 399-409 ◽  
Author(s):  
Gregory H. Leonard ◽  
Patricia J. Langhorne ◽  
Michael J.M. Williams ◽  
Ross Vennell ◽  
Craig R. Purdie ◽  
...  

AbstractHere we describe the evolution through winter of a layer of in situ supercooled water beneath the sea ice at a site close to the McMurdo Ice Shelf. From early winter (May), the temperature of the upper water column was below its surface freezing point, implying contact with an ice shelf at depth. By late winter the supercooled layer was c. 40 m deep with a maximum supercooling of c. 25 mK located 1–2 m below the sea ice-water interface. Transitory in situ supercooling events were also observed, one lasting c. 17 hours and reaching a depth of 70 m. In spite of these very low temperatures the isotopic composition of the water was relatively heavy, suggesting little glacial melt. Further, the water's temperature-salinity signature indicates contributions to water mass properties from High Salinity Shelf Water produced in areas of high sea ice production to the north of McMurdo Sound. Our measurements imply the existence of a heat sink beneath the supercooled layer that extracts heat from the ocean to thicken and cool this layer and contributes to the thickness of the sea ice cover. This sink is linked to the circulation pattern of the McMurdo Sound.


2015 ◽  
Vol 9 (11) ◽  
pp. 2537-2540 ◽  
Author(s):  
Christiane Uhlig ◽  
Fabian Kilpert ◽  
Stephan Frickenhaus ◽  
Jessica U Kegel ◽  
Andreas Krell ◽  
...  

2018 ◽  
Author(s):  
Daniel Price ◽  
Iman Soltanzadeh ◽  
Wolfgang Rack

Abstract. Knowledge of the snow depth distribution on Antarctic sea ice is poor but is critical to obtaining sea ice thickness from satellite altimetry measurements of freeboard. We examine the usefulness of various snow products to provide snow depth information over Antarctic fast ice with a focus on a novel approach using a high-resolution numerical snow accumulation model (SnowModel). We compare this model to results from ECMWF ERA-Interim precipitation, EOS Aqua AMSR-E passive microwave snow depths and in situ measurements at the end of the sea ice growth season. The fast ice was segmented into three areas by fastening date and the onset of snow accumulation was calibrated to these dates. SnowModel falls within 0.02 m snow water equivalent (swe) of in situ measurements across the entire study area, but exhibits deviations of 0.05 m swe from these measurements in the east where large topographic features appear to have caused a positive bias in snow depth. AMSR-E provides swe values half that of SnowModel for the majority of the sea ice growth season. The coarser resolution ERA-Interim, not segmented for sea ice freeze up area reveals a mean swe value 0.01 m higher than in situ measurements. These various snow datasets and in situ information are used to infer sea ice thickness in combination with CryoSat-2 (CS-2) freeboard data. CS-2 is capable of capturing the seasonal trend of sea ice freeboard growth but thickness results are highly dependent on the assumptions involved in separating snow and ice freeboard. With various assumptions about the radar penetration into the snow cover, the sea ice thickness estimates vary by up to 2 m. However, we find the best agreement between CS-2 derived and in situ thickness when a radar penetration of 0.05-0.10 m into the snow cover is assumed.


Elem Sci Anth ◽  
2021 ◽  
Vol 9 (1) ◽  
Author(s):  
Caroline Jacques ◽  
Célia J. Sapart ◽  
François Fripiat ◽  
Gauthier Carnat ◽  
Jiayun Zhou ◽  
...  

We report on methane (CH4) stable isotope (δ13C and δ2H) measurements from landfast sea ice collected near Barrow (Utqiagvik, Alaska) and Cape Evans (Antarctica) over the winter-to-spring transition. These measurements provide novel insights into pathways of CH4 production and consumption in sea ice. We found substantial differences between the two sites. Sea ice overlying the shallow shelf of Barrow was supersaturated in CH4 with a clear microbial origin, most likely from methanogenesis in the sediments. We estimated that in situ CH4 oxidation consumed a substantial fraction of the CH4 being supplied to the sea ice, partly explaining the large range of isotopic values observed (δ13C between –68.5 and –48.5 ‰ and δ2H between –246 and –104 ‰). Sea ice at Cape Evans was also supersaturated in CH4 but with surprisingly high δ13C values (between –46.9 and –13.0 ‰), whereas δ2H values (between –313 and –113 ‰) were in the range of those observed at Barrow. These are the first measurements of CH4 isotopic composition in Antarctic sea ice. Our data set suggests a potential combination of a hydrothermal source, in the vicinity of the Mount Erebus, with aerobic CH4 formation in sea ice, although the metabolic pathway for the latter still needs to be elucidated. Our observations show that sea ice needs to be considered as an active biogeochemical interface, contributing to CH4 production and consumption, which disputes the standing paradigm that sea ice is an inert barrier passively accumulating CH4 at the ocean-atmosphere boundary.


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