Polonium-210 and lead-210 in Antarctic marine biota and sea water

Concentrations of the naturally-ocurring radionuclides ²¹⁰Po and ²¹⁰Pb were measured in krill (Euphausia superba), mesozooplankton, phytoplankton and sea water collected during the South African SIBEX cruise to the Antarctic in autumn 1984. The data reported constitute the first substantial measurements on ²¹⁰Po and ²¹⁰Pb in such samples in the Antarctic Ocean. The concentrations of ²¹⁰Po in mesozooplankton and phytoplankton are unexceptional in comparison with those from other oceans. The SIBEX E. superba, however, have higher levels of ²¹⁰Po than usually found in euphausiids. The ²¹⁰Po data, combined with reasonable estimates of biological quantitites such as the fractional assimilation, are used to obtain information about the diet of E. superba. It is suggested that the higher ²¹⁰Po in the SIBEX E. superba reflects a change from an almost entirely phytoplanktonic diet in summer to a more omnivorous diet as winter approaches. The data show that there are allometric relationships between the ²¹⁰Po content of euphausiids and animal size; these are discussed briefly. The limited sea-water data presented are characterized by unusually high ²¹⁰Po:²¹⁰Pb activity ratios and need further investigation.     

Polonium-210 and lead-210 in marine food chains

²¹⁰Po and ²¹⁰Pb have been measured systematically in whole animals, muscle and hepatopancreas of crustaceans and of molluscan cephalopods representative of a pelagic and benthic food chain. The same nuclides were also measured in liver, pyloric caecum, stomach contents and muscle of tuna. The concentration factors from sea water to whole animals were approximately constant along both food chains, being of the order of 10⁴ for ²¹⁰Po and 10² for ²¹⁰Pb. The highest concentration factors were found in shrimp of the genus Sergestes. In muscle, the concentration factors were an order of magnitude less; in the hepatopancreas, they were an order of magnitude higher, reaching 10⁶ in shrimp of the genus Sergestes. Such concentrations imply alpha-radiation doses of the order of 10 rem per year and more in this organ, which contains about 50 to 90% of the ²¹⁰Po in the whole animal in the 11 species analyzed. A detailed study of the intracellular behaviour of ²¹⁰Po in the hepatopancreas is clearly indicated. ²¹⁰Po can be used as a sensitive natural tracer in biological systems. Thus, feeding Meganyctiphanes norvegica in the laboratory on food low in ²¹⁰Po led to an approximate value of about 61/2 days for the biological half-life of ²¹⁰Po in the hepatopancreas of this euphausiid. Furthermore, the data on ²¹⁰Po and ²¹⁰Pb in the cephalopod hepatopancreas allowed the time of conservation of frozen squid which had been bought at the market to be estimated.     

210Po and 210Pb in zooplankton fecal pellets

²¹⁰Po and ²¹⁰Pb concentrations in fecal pellets from the zooplanktonic euphausiid Meganyctiphanes norvegica are reported. The ²¹⁰Po:²¹⁰Pb activity ratio is 2.2±0.3, a value in good agreement with that found in suspended particulate matter in surface seawater. Estimates of ²¹⁰Po and ²¹⁰Pb removal times from the mixed layer by fecal pellets alone yield values which are of the same order of magnitude as the removal times for these nuclides by all routes. It is suggested that there is a high probability that zooplanktonic fecal pellets play a significant role in the removal of both these nuclides from the surface layers of the ocean.     

Flux of cadmium through euphausiids

Flux of the heavy metal cadmium through the euphausiid Meganyctiphanes norvegica was examined. Radiotracer experiments showed that cadmium can be accumulated either directly from water or through the food chain. When comparing equilibrium cadmium concentration factors based on stable element measurements with those obtained from radiotracer experiments, it is evident that exchange between cadmium in the water and that in euphausiid tissue is a relatively slow process, indicating that, in the long term, ingestion of cadmium will probably be the more important route for the accumulation of this metal. Approximately 10% of cadmium ingested by euphausiids was incorporated into internal tissues when the food source was radioactive Artemia. After 1 month cadmium, accumulated directly from water, was found to be most concentrated in the viscera with lesser amounts in eyes, exoskeleton and muscle, respectively. Use of a simple model, based on the assumption that cadmium taken in by the organism must equal cadmium released plus that accumulated in tissue, allowed assessment of the relative importance of various metabolic parameters in controlling the cadmium flux through euphausiids. Fecal pellets, due to their relatively high rate of production and high cadmium content, accounted for 84% of the total cadmium flux through M. norvegica. Comparisons of stable cadmium concentrations in natural euphausiid food and the organism's resultant fecal pellets indicate that the cadmium concentration in ingested material was increased nearly 5-fold during its passage through the euphausiid. From comparisons of all routes by which cadmium can be released from M. norvegica to the water column, it is concluded that fecal pellet deposition represents the principal mechanism effecting the downward vertical transport of cadmium by this species.     

Assimilation of 210Po by the mussel Mytilus edulis from the alga Isochrysis galbana

Marine invertebrates are thought to accumulate ²¹⁰Po primarily from their food. In this study, a pulse-chase methodology was used to examine the assimilation and depuration of ²¹⁰Po by Mytilus edulis from the common marine alga Isochrysis galbana. The digestion of ²¹⁰Po from I. galbana occurred via a biphasic process, characteristic of a rapid (extracellular) and slow (intracellular) digestion typical of marine bivalves. The mantle/gill and foot have no known digestive role, yet their ²¹⁰Po specific activities increased after 24 h. It is proposed that this increase in ²¹⁰Po specific activity was related to ²¹⁰Po being incorporated into these tissues from ²¹⁰Po assimilated from I. galbana during extracellular digestion. It is proposed that the linear loss of ²¹⁰Po previously accumulated by control mussels was related to the continual state of renewal and replacement of cellular proteins, with ²¹⁰Po turnover and metabolism governed by protein turnover and metabolism. M. edulis' assimilation efficiency of ²¹⁰Po from the ²¹⁰Po-labelled alga was calculated to be 17.2 ± 2.1%, and thus similar to that of Ag, Cd, Co, Se and Zn by bivalves from other marine algae species. It is proposed that the assimilation efficiency of ²¹⁰Po is a function of protein assimilation. Received: 27 August 1998 / Accepted: 3 September 1999     

210Pb as a dietary indicator in the Antarctic pelagic community

The naturally occurring radionuclide ²¹⁰Po is useful as a tracer of diets of marine organisms. Data for ²¹⁰Pb, the grandparent of ²¹⁰Po, are less abundant: we therefore report here ²¹⁰Pb concentrations in a substantial collection of marine biota obtained from the Antarctic Ocean during the SIBEX II cruise in 1985. The general levels of ²¹⁰Pb are within the range of previously published data but, as in the case of ²¹⁰Po, there are differences which can be associated with variations in the diet of the organism. The levels of ²¹⁰Pb in the krill Euphausia superba show seasonal changes which can be interpreted in terms of changing diet. In a simple classification of the pelagic food chain, the levels of ²¹⁰Pb tend to increase from omnivores to filter-feeders to predators.     

Polonium-210 content of marine shrimp: Variation with biological and environmental factors

The concentrations of ²¹⁰Po and ²¹⁰Pb were determined in more than 30 species of marine shrimp. Samples were collected in the years 1977 to 1980; most were from the Mediterrancean Sea near Monaco, the remainder from Kuwait, South Africa, USA and Great Britain. The median ²¹⁰Po concentration was 8.0 pCi g^-1 dry wt in the whole shrimp and 85 pCi g^-1 dry in the hepatopancreas; the corresponding ²¹⁰Po:²¹⁰Pb activity ratios were 77 and 138, respectively. The range of concentrations covered more than two orders of magnitude for both nuclides. The variations in the levels of ²¹⁰Po, in particular, could be related to biological and environmental factors; thus, penaeid shrimp had ²¹⁰Po at median concentrations some three to four times higher than carid shrimp, and there was a steady increase in the median ²¹⁰Po concentration as one moved from estuarine to coastal to pelagic to deep-pelagic species. ²¹⁰Po levels were highest in 3 species of deep-pelagic penaeids, where a median ²¹⁰Po concentration in the whole shrimp of 43 pCi g^-1 dry wt was found. The natural radiation dose received by the hepatopancreas of such individuals will be of the order of 100 rem per yr. Elevated ²¹⁰Po was also found in 4 species collected near Kuwait. The ²¹⁰Po data are interpreted as indicating changes in the food regime of different shrimp; specifically it is suggested that ²¹⁰Po-rich items such as hepatopancreas, faecal pellets and organic particulates are likely to be important in the diet of shrimp which feed at depth in the ocean. It is suggested further that the ultimate availability of ²¹⁰Po to the foodchain depends on its form in sea water, and the need for information concerning the degree of organic binding of ²¹⁰Po in natural waters in stressed.     

Predation on euphausiids by cod,Gadus morhua,in winter in Icelandic subarctic waters

The euphausiids consumed by cod (Gadus morhua Linnaeus, 1758) taken in November 1983 and February–March 1984 on feeding grounds in the subarctic shelf area north-west, north-east, and south-east of Iceland have been examined. A total of 2 714 euphausiids occurred in the 1 029 stomachs with food which were analysed; of these 1 640 (60%) could be identified to species. Thysanoëssa inermis (Krøyer, 1846) and Meganyctiphanes norvegica (M. Sars, 1857) were most numerous, constituting 58 and 40%, respectively, of the euphausiids which could be identified. The other euphausiids were, in declining numbers of abundance, T. raschii (M. Sars, 1864), T. longicaudata (Krøyer, 1846), and Nematoscelis megalops G. O. Sars, 1883. The mean number of euphausiids occurring per stomach showed considerable variation between both sampling areas and time of sampling. In each area, the mean number of M. norvegica occurring per stomach was similar at both sampling times, while for T. inermis it was greater in February–March than in November. The mean number of euphausiids occurring per stomach increased with increasing size of cod, being 1 to 2 and 4 to 6 in 10 to 30 cm and 50 to 70 cm cod, respectively. An examination of the diel variation in the occurrence of the euphausiids in the stomachs indicated two peaks, one in the morning before sunrise and another in the evening around and after sunset.     

Turnover and vertical transport of zinc by the euphausiid Meganyctiphanes norvegica in the Ligurian Sea

Participatory turnover time is defined as the time required to cycle an element in a system through a given material in that system. The participatory turnover time of ionic zinc by the adult Meganyctiphanes norvegica population in the Ligurian Sea ranged between 498 and 1243 years, depending upon the available food supply, and considering the food chain as the only route for zinc accumulation by the population. A total-impact turnover time was calculated as the sum of the participatory turnover time for live individuals plus the time required for dead euphausiids to lose 90% of their zinc to the water. Carcasses lost zinc to the water slower than either feces or molts, and so established the maximum loss time for all particulate excretion products; nevertheless, total-impact turnover time for zinc did not differ significantly from the participatory turnover time. The net vertical transport of zinc by M. norvegica from the sea surface to any specified depth can be calculated as the sum of the dissolved zinc excreted below the depth plus the concentrations of zinc left in feces, molts, and carcasses after they have sunk to the specified depth. Carcasses sink the fastest and lose the smallest fraction of their zinc concentration during descent; fecal pellets sink the slowest and lose the greatest fraction of their zinc concentration, and molts are intermediate. Nevertheless, feces represents the major route for delivering zinc to the bottom of the Ligurian Sea (2500 m), because concentration of the element in the pellets is so much higher than in carcasses or molts. Excretion of dissolved zinc into the water at the vertical migration depth of the living population during daylight hours was also inconsequential. Feces zinc represented over 80% of the total zinc transported to the sea floor if only marginal food supplies were available to the euphausiids, and over 90% if food was in sufficient supply. M. norvegica can effect a net transport of about 98% of its body zinc concentration below 500 m daily, in conditions of sufficient food supply and assuming that no released products are eaten during descent. If the food supply in the Ligurian Sea is considered only marginal throughout the year, M. norvegica can still effect a daily net transport below 500 m of about 36% of its body concentration, and about 6% of its body concentration will reach 2500 m daily.     

Flux of 141Ce through a euphausiid crustacean

The role of the Mediterranean euphausiid Meganyctiphanes norvegica in the cycling of radiocerium (¹⁴¹Ce) was examined. When uptake of ¹⁴¹Ce occurs directly from the water, a dynamic population equilibrium is reached at a concentration factor of about 250. Molting was responsible for up to 99% loss of total body burden at first molt, and about 45% of the remaining activity at second molt, thus denying true longterm equilibrium to individual animals. Fecal pellets did not contain measureable ¹⁴¹Ce activity when the euphausiids accumulated the isotope from water, thus proving that surface adsorption was the key accumulating process from water. When radiocerium was taken in through ingestion of labelled Artemia, about 99% of the body burden was voided as fecal pellets. Excretion by this route was accelerated when euphausiids were fed non-radioactive Artemia during loss phase. Radioactive counts of the pellets confirmed that all ingested ¹⁴¹Ce was lost through defecation. When ¹⁴¹Ce was ingested as labelled phytoplankton, a substantial fraction of the total body burden occurred in the molts, which indicated that the phytoplankton lost ¹⁴¹Ce to the water and the radioactivity was subsequently adsorbed to outer surfaces of the euphausiids. Molts, fecal pellets, and freshly-killed euphausiids lost ¹⁴¹Ce to the water exponentially, the rates being similar to the exponential portions of the loss curves for live, non-molting individuals. It is suggested that M. norvegica, and probably other pelagic zooplankters, can greatly accelerate radiocerium transport to the ocean floor by packaging the isotope as fecal pellets. In coastal areas subject to low-level radioactive waste disposal, ¹⁴¹Ce might be ionic (or at least soluble) to a great extent, in which case euphausiids could take up the isotope rapidly and accelerate its vertical transport via molting.     

Effect of Cd on accumulation and loss of 210Po in the mussel Mytilus edulis

As a result of ²¹⁰Po's previously identified association with sulphur-rich proteins, metallothioneins could have a significant effect on the behaviour and fate of ²¹⁰Po in molluscs. Starved control and cadmium-exposed mussels, Mytilus edulis, were fed ²¹⁰Po-labelled algae (Isochrysis galbana) for 5 d and then allowed to depurate in clean sea water. Cadmium-exposed M. edulis accumulated less ²¹⁰Po in the digestive gland and the remainder of the tissue than control mussels, although this was due to a decrease in tissue weight. More than 40% of ²¹⁰Po was identified as being associated with high molecular weight and heat-treated cytosol proteins in M. edulis. Mussels in a starved state are known to recycle as much as 90% of their amino acids. It is proposed that ²¹⁰Po associated with these and other proteins is recycled, explaining why no significant loss of ²¹⁰Po was observed from the remainder of the tissue in either control or Cd-exposed mussels. Cadmium-induced metallothioneins had no effect on the distribution of ²¹⁰Po in M. edulis; <5% associated with the cytosolic fraction was considered to principally contain metallothioneins. It is suggested that ²¹⁰Po's apparent relationship with metallothioneins is coincidental rather than connected with its role in the regulation of metals. Received: 30 March 1998 / Accepted: 3 August 1998     

Diel vertical migrations and nocturnal feeding of a dense coastal krill scattering layer (Thysanoessa raschi and Meganyctiphanes norvegica) in stratified surface waters

To study the nocturnal feeding of euphausiids during vertical migrations and its impact on the phytoplankton, a phytoplankton-rich water mass (drogue marked) drifting over a dense krill scattering layer (acoustic 104kHz) in the lower St. Lawrence estuary was monitored over 46 h in July 1982. Phytoplankton >20 m was abundant and mostly concentrated at the bottom of the photic layer above the pycnocline. Less than 42% of the particulate carbon was due to phytoplankton. The krill scattering layer was about 2 to 3 km in width, elongated along the 100-m bathymetric contour, and absent when the bottom was shallower than 50 m. Its upper day depth was 50 m. At deeper depths, its vertical distribution frequently changed from unimodal to polymodal shapes and viceversa, often with large concentrations of zooplankton just above the bottom. Typical vertical migrations were observed on both days. At night the scattering layer had a lower scattering strength. Most of it was below the thermocline but net catches showed that large concentrations of euphausiids (up to 57 individuals m^-3) crossed it. Stomach pigment content of Thysanoessa raschi was generally low, but mean stomach fullness was always high. They were more opportunistic than herbivorous. From stomach fullness and the presence of a food bolus in mouth parts, feeding in surface waters appeared to be intensive, but gut content indicated that food was not processed there. It is therefore suggested that individuals underwent vertical interchanges across the thermocline while feeding during the night. Meganyctiphanes norvegica had significant herbivorous activity during the night. The grazing pressure impact of the scattering layer on phytoplankton was negligible.Contribution to the program of GIROQ (Groupe interuniversitaire de recherches océanographiques du Québec)     

Flux of different forms of 106Ru through a marine zooplankter

The dynamics of accumulation and loss of different physico-chemical forms of ¹⁰⁶Ru were measured in the euphausiid Meganyctiphanes norvegica. The accumulation of ¹⁰⁶Ru was directly related to the concentration of the radioisotope in solution, as evidenced by similar concentration factors for euphausiids in the low and high activity ¹⁰⁶Ru chloride solutions. The chemical form of the radioisotope in solution had a pronounced effect on the uptake, with ¹⁰⁶Ru chloride fractions being accumulated at a faster rate than ¹⁰⁶Ru nitrosyl-nitrato complexes. Euphausiids lost ¹⁰⁶Ru, previously accumulated from the ¹⁰⁶Ru chloride complexes, at a faster rate than ¹⁰⁶Ru which had been accumulated from ¹⁰⁶Ru nitrosyl-nitrato forms. Also, in the case of the ¹⁰⁶Ru chloride complexes, the loss rate was inversely proportional to the time allowed for isotope accumulation. The process of molting greatly accelerated the loss of ¹⁰⁶Ru from euphausiids, with first molts shed during the loss phase accounting for 70 to 80% of the total ¹⁰⁶Ru body burden. When euphausiids accumulated ¹⁰⁶Ru from the food chain, the initial-loss rate was rapid due to large amounts of the radioisotope associated with fecal pellets; however, no relationship was found between loss rate and the number of food rations received. Molts from these individuals did not contain ¹⁰⁶Ru, thus, loss from euphausiids obtaining this radioisotope through the food chain is mainly due to fecal pellet deposition and other excretion or exchange processes.     

In vivo accumulation of radioactive polonium by the giant kelp Macrocystis pyrifera

The in vivo accumulation rate of ²¹⁰Po by Macrocystis pyrifera (L) Ag. has been determined by the tagging of specific parts of young, growing lamina in La Jolla kelp beds and their subsequent collection for ²¹⁰Po analysis. The rates of accumulation for observed and growth-corrected data were, respectively, 0.78x10^-9 pCi/cm² sec (1.73x10^-9 dpm/cm² sec) and 1.17x10^-9 pCi/cm² sec (2.60x10^-9 dpm/cm² sec). Invert, but biologically foulable, glass-slide surfaces exposed to the kelp bed environment yielded ²¹⁰Po accumulation rates of 0.64x10^-9 pCi/cm² sec (1.42x10^-9 dpm/cm² sec), slightly less than those of M. pyrifera. Distinction is made between observed net accumulation rate and gross rates or total flux. Several factors contributing to the final net accumulation rate are discussed.     

Observations sur le développement larvaire de Meganyctiphanes norvegica (Crustacea: Euphausiacea) au laboratoire

Larvae of Meganyctiphanes norvegica (M. Sars), caught with a plankton net, were reared in the laboratory from the calyptopis phase onwards, under different temperature and trophic conditions. Eyestalk ablation was performed on the first furciliae. Data are presented on growth, moulting rate and ontogenesis of the larvae as a function of the varying experimental conditions, and on larval morphology, pigmentation and diet. Recent modifications of larval nomenclature in euphausiids are discussed.

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Observations sur le développement larvaire de Meganyctiphanes norvegica (Crustacea: Euphausiacea) au laboratoire

     

Timing of septal formation in two species of Nautilus based on radiometric and aquarium data

Growth rates of four Nautilus scrobiculatus Lightfoot and three N. pompilius Linnaeus captured in Papua New Guinea in 1985 were measured using a chronology based on the naturally occurring radionuclides ²¹⁰Pb and ²¹⁰Po. The age of the las septum in mature specimens of both species was more than one year, whereas the time of septal formation in a submature specimen of N. pompilius was ca 180 d. The ²¹⁰Po/²¹⁰Pb method was also used to determine the growth rates of four immature N. pompilius captured in the Philippines in 1983 before and after introduction into an aquarium. Introduction into the aquarium was marked by a dramatic decrease in the activity of ²¹⁰Pb of the septa, the formation of a black line on the exterior of the shell, and a reduction in the spacing of adjacent septa in two specimens. Based on the number of septa formed in the aquarium, the average time of septal formation ranged from 50 to 80 d. These estimates were consistent with those calculated from the ²¹⁰Po/²¹⁰Pb activity ratios of the septa that formed in the aquarium, thus providing a check on the radiometric method. The average time of septal formation just prior to introduction into the aquarium appears, within the uncertainty of the radioactive measurements, to have been similar to that in the aquarium, indicating no dramatic alteration in the growth rate of these specimens.     

Effects of temperature and size on molting of euphausiid crustaceans

The effects of temperature and body size on the intermolt periods (molting frequencies) of the North Pacific euphausíid Euphausia pacifica and the Mediterranean forms of Meganyctiphanes norvegica, Euphausia krohnii, Nematoscelis megalops, and Nyctiphanes couchii were studied under controlled conditions in the laboratory. Mean intermolt periods for E. pacifica and M. norvegica were inversely and linearly related to temperature, over temperature ranges which the euphausiids normally encounter in the sea. At higher temperatures there was a tendency for three size groups of M. norvegica to approach a minimum intermolt period independent of temperature. M. norvegica cycled for different time periods between 13° and 18°C molted regularly at mean frequencies which would be expected if the animals had been held constantly at the timeweighted means of the two experimental temperatures. The increase in mean intermolt period per unit weight was faster in small, fast-growing M. norvegica than in large, slow-growing adults. This relationship was corroborated by following the changes in the intermolt period of an actively growing individual N. couchii over an 11 month period. Neither feeding nor the time of year of collection affected the molting frequency as long as temperature and animal weight were held constant. No tendency was found for euphausiids of the same species and/or size, and from the same collection, to molt on the same night. Molting occurred at night 80 to 90% of the time for all species, over the temperature ranges normally experienced by the euphausiids in the sea, and over all animal weights tested. There appeared to be a weakening of the night-time molting rhythm at low temperatures. Although neither temperature nor anímal weight substantially affected the night-time molting rhythm, both affected the mean intermolt period. Therefore, both temperature and body size apparently act together to adjust the length of the intermolt period of each individual in increments of whole days, but they exert little control over time of molting within any 24h period. No information was obtained regarding the factors which specify night-time molting over daytime molting within any 24 h period; however, regulation of certain hormone activities is probably involved.     

Ecology of the euphausiidsThysanoessa raschi,T. inermis andMeganyctiphanes norvegica in Ísafjord-deep,northwest-Iceland

The seasonal abundance, distribution, maturity, growth and population dynamics of the euphausiidsThysanoessa raschi (M. Sars, 1864),T. inermis (Krøyer, 1846) andMeganyctiphanes norvegica (M. Sars, 1857) were studied in Ísafjord-deep, a fjord in northwest Iceland, from February 1987 to February 1988. Sampling was made at nine stations along the length of the fjord at approximately monthly intervals, along with hydrographic measurements and water sampling for nutrient analysis and measurements of chlorophylla concentrations. Spring warming of the water began in late May and maximum temperatures (8° to 10°C) were observed in late July–September. The phytoplankton spring-bloom started in early April, and the highest chlorophylla levels were measured in early May (7.0 mg m^–3). A small increase was observed in the chlorophylla content in August. The greatest abundance of juveniles and males and females of all three species was observed during January and February 1988, during which period the euphausiids were concentrated in the middle and inner parts of the fjord. Euphausiid eggs were first recorded in the plankton in mid-May, and the greatest abundance ofThysanoessa spp. larvae occurred at the end of May. Larvae ofM. norvegica were not observed in Ísafjord-deep, indicating that recruitment of this species was occurring from outside the fjord.T. raschi andT. inermis had a life span of just over 2 yr; the life span ofM. norvegica was more difficult to determine. Almost all femaleT. raschi were mature at the age of 1 yr, while mostT. inermis females appeared not to mature until 2 yr of age. Most males of both species took part in breeding at 1 yr of age. The maximum carapace length ofT. raschi andT. inermis was 8 to 9 and 9 to 10 mm, respectively. The largestM. norvegica had a carapace length of 9 to 10 mm. The spawning of the euphausiids in Ísafjord-deep appeared to be closely related to the phytoplankton spring bloom; water temperature appeared to have no influence on spawning.     

Microsetella norvegica: a rare report of a potentially abundant copepod on the Scotian Shelf

Fine mesh (0.080 mm) zooplankton samples were collected along an onshore-offshore transect during three cruises (February to May, 1983) off southwest Nova Scotia, Canada. The small harpacticoid copepod Microsetella norvegica was numerically the dominant copepod during the winter (February) cruise, where it composed up to 50% of the total zooplankton, and was consistently among the three most abundant copepods during the spring cruises. Due to its small size (<0.45 mm in length), M. norvegica has rarely been reported from plankton surveys of the northwest Atlantic. However, existing reports indicated it varies interannually from being a rare to an abundant member of the zooplankton community in the northwest Atlantic.     

Interactions of marine plankton with transuranic elements

In a series of laboratory experiments, the biokinetics of ²⁴¹Am, an important transuranium element, was studied in Meganyctiphanes norvegica, a euphausiid common in the northwestern Mediterranean. The euphausiids accumulated Am from water by passive adsorption onto exoskeletons, achieving wet weight concentration factors on the order of 10² after 1 wk exposure; concentration factors varied inversely with the size of the euphausiids and linearly with their surface area:wet weight ratios. Essentially all (96±10%) of the Am taken up from water was associated with the exoskeleton, so that negligible Am was retained by the euphausiids after molting. The retention half-time of Am in molts was 2.9 d. Euphausiids could also concentrate Am from feeding suspensions by ingesting Am-labelled diatom cells, although there was negligible Am assimilation (3±2% after 4 d feeding); after passage through the gut, virtually all (99%) of the ingested Am was defecated within 1 wk. The retention half-time of Am in fecal pellets was 41 and 51 d at 13° and 5°C, respectively. In oceanic waters, where the preponderance of ²⁴¹Am is in the dissolved phase, uptake of Am from water by euphausiids would be the dominant route of bioaccumulation. The results underscore the importance of sinking biogenic debris from zooplankters in mediating the vertical transport of Am in the sea. Given their retention half-times for ²⁴¹Am and their rapid sinking rates, fecal pellets and discarded molts have the potential to deliver most of their Am to the sediments.