genetic variability of the metridia lucens complex (copepoda) in the southern ocean
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Genetic variability of the Metridia lucens complex (Copepoda) in the SouthernOcean
Alexandra N. Stupnikova, Tina N. Molodtsova, Nikolay S. Mugue, Tatyana V.Neretina
PII: S0924-7963(13)00106-1DOI: doi: 10.1016/j.jmarsys.2013.04.016Reference: MARSYS 2367
To appear in: Journal of Marine Systems
Received date: 16 September 2012Revised date: 24 April 2013Accepted date: 27 April 2013
Please cite this article as: Stupnikova, Alexandra N., Molodtsova, Tina N., Mugue,Nikolay S., Neretina, Tatyana V., Genetic variability of the Metridia lucens com-plex (Copepoda) in the Southern Ocean, Journal of Marine Systems (2013), doi:10.1016/j.jmarsys.2013.04.016
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Genetic variability of the Metridia lucens complex (Copepoda) in the Southern Ocean
Alexandra N. Stupnikova1, Tina N. Molodtsova
1, Nikolay S. Mugue
2 and Tatyana V. Neretina
3
1 P.P.Shirshov Institute of Oceanology Russian Academy of Science, 36, Nahimovsky prospect,
Moscow, 117997, RF
2 Russian Federal Research Institute of Fisheries and Oceanography, 17, Krasnoselskaya street,
Moscow, 107140, RF.
3 White Sea Biological Station, Department of Biology Lomonosov Moscow State University,
a/ya 20, Glavpochtamt, Kandalakshsky raion, Murmanskaya oblast, 184042, RF.
Correspondence: Alexandra Stupnikova, Fax: +7(499)1245983, E-mail:
Running title: Genetic variability of Metridia lucens
Abstract
Analysis of the fragment of the mtDNA gene СО1 has revealed two genetically distinct
groups of the Metridia lucens complex in the South part of the Atlantic. While the intragroup
polymorphism was less than 1%, the intergroup difference was about 9.5%. These two groups
may be considered as representing two cryptic species within the M. lucens complex: M. lucens
North and M. lucens South. These forms are found mainly to the North and to the South of the
South Polar Front. The results are confirmed by an analysis of the nuclear rDNA ITS1-5,8S-ITS2
fragment. No hybrids between the two forms were detected. M. lucens North inhabits the waters
> 4°C that allow us to discuss the temperature as putative limiting factor for the distribution.
Keywords: plankton, Copepoda, cryptic species, Metridia lucens, genetic diversity, the Southern
Ocean
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1. Introduction
Spatial irregularities in the distribution of planktonic organisms observed in the Southern
Ocean substantially agree with patterns of fronts separating different Antarctic water masses
(Maslennikov, 1994; Read et al., 2002). According to the modern biogeographic classification of
pelagic ecosystems (Errhif et al., 1997; Longhurst, 1998) the Polar Front is the biogeographical
boundary separating Subantarctic and Antarctic biogeographical provinces. The Polar Frontal
Zone is also viewed as a separate province (Longhurst, 1998) inhabited by species from both
adjacent provinces.
The transfrontal water exchange explains the fact that a number of zooplankters (e.g.,
dominant copepods Calanus simillimus, Ctenocalanus citer, Rhincalanus gigas and Metridia
lucens) inhabit all hydrological zones of the Southern Ocean (South Atlantic Zooplankton, 1999).
However, some reports provide evidence for a restricted gene flow between populations
separated by the fronts and for a maintaining of isolated populations (Bucklin et al., 1996, 2000;
Goetze, 2005).
Genetic methods provide alternative or additional means of identifying known species.
Genetic analysis of the region of mitochondrial cytochrome oxidase I (mtCOI) has been widely
used to discriminate species throughout the animal kingdom (Hebert et al., 2003), including
Crustacea (Costa et al., 2007) and in particularly Copepoda (Bucklin et al., 2010). The nuclear
rDNA fragment internal transcribed spacer (ITS) has also been used as a successful marker for
phylogenetic and population analysis in crustaceans (Chu et al., 2001), including copepods
(Elvers et al., 2006; Ki et al., 2009).
Metridia lucens Boeck, 1865 (Copepoda: Calanoida) is a widely distributed dominant
interzonal species (Vervoort, 1957) characterized by a high morphological variability (Bradford-
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Grieve, 1999). It is shown to be an important member of the zooplankton of all open oceanic
regions of the World Ocean, except for the high Arctic.
The aim of this work is to evaluate the degree of genetic isolation of M. lucens populations
inhabiting different hydrological zones of the Southern Ocean based on mitochondrial (COI) and
nuclear (ITS) DNA fragments.
2. Materials and Methods
2.1. Sample collection
The specimens of the M. lucens complex was collected during the Southern Hemisphere
Summer (December 2009 - January 2010) from seven stations and during the Antarctic Spring
(October-November 2010) from 22 stations along the Eastern and Western (The Drake Passage)
sections of the Atlantic sector of the Southern Ocean (Fig. 1, Table 1). The distance between the
sampling sections was 3-4 thousand kilometers. Each sampling location represented a separate
hydrological zone: the Subantarctic Zone (SAZ), the Polar Frontal Zone (PFZ), the Antarctic
Zone (AZ), with additional sampling in the Subtropical Zone (STZ).
Each sample was collected with a Juday net from the water layer 0-300 m. Immediately
after collection, adults of the M. lucens complex were isolated from the samples. The specimens
were identified by the morphological traits (Bradford-Grieve, 1994; Bradford-Grieve et al.,
1999). In total, 89 individuals were collected.
Water temperature and salinity were measured with CTD SeaВird 911+ probe at the
moment of sampling. Vertical profile of temperature and salinity was used to locate the ACC
hydrological boundaries (Sokolov and Rintoul, 2002, 2009). Exact zone boundaries were
evaluated based on the current velocity registered by SADCP (RDI Ocean Surveyor).
For comparison, four specimens of the M. lucens s.s. Boeck, 1865 from the North Sea have
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also been used in this study. They were collected at Marine Biological Station, Espeland, in the
Raunefjord, 20 km South from Bergen.
2.2. DNA Amplification and Sequencing.
Promega Wizard SV Genomic DNA Purification Kit (Promega Corporation, Madison,
USA) was used for tissue lysis and DNA purification following the manufacturer's protocol.
Polymerase chain reaction (PCR) amplification of nuclear ITS1-5.8S rDNA-ITS2 region
was accomplished with the primers LR1 (GGTTGGTTTCTTTTCCT) and SR6R
(AAGWAAAAGTCGTAACAAGG) (Gardes and Bruns, 1993). This 487bp nuclear region
comprises a partial sequence of the 18S rRNA gene, complete sequences of the ITS1, 5.8S rRNA
and ITS2 and a partial sequence of the 28S rRNA gene. PCR amplification of the 535bp fragment
of the mtCOI gene was performed with the universal primers LCOI 1490
(GGTCAACAAATCATAAAGATATTGG) and HCOI 2198
(TAAACTTCAGGGTGACCAAAAAATCA) (Folmer et al., 1994). Loci were amplified using
Encyclo PCR kit (Evrogen Joint Stock Company, Russia). Amplification was done in a total
volume of 25 ml reaction mix containing 1 X PCR buffer, 1 µL of 10 µM of primer pair mix, 1
µL of the template, 0.2 mM of each dNTP and 0.5 units Taq polymerase. Reactions mixtures
were heated to 94°C for 120 s, followed by 35 cycles of 15 s at 94°C, 30 s at a specific annealing
temperature and 60 s at 72 °C, and then the final extension of 7 min at 72°C on Veriti® Thermal
Cycler. Annealing temperature was set to 45° C for the CO1 and 52°C for the ITS1-5.8S rDNA-
ITS2 primer pairs. The Promega PCR Purification Kit protocol (Promega) was employed to
purify amplification products. Amplification products were sequenced in both directions. Each
sequencing reaction mixture, including 1 мl BigDye3.1 (Applied Biosystems, Perkin-Elmer
Corporation, Foster City, CA), 1 мl of 1 µM primer and 1µL of DNA template, ran for 40 cycles
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at 96°C (15 s), 50°C (30 s) and 60 °C (4 min). Sequences were purified by ethanol precipitation
to remove unincorporated primers and dyes. Products were re-suspended in 12 µl formamide and
electrophoresed in an ABI Prism_ 3500 sequencer (Applied Biosystems).
The obtained sequences were submitted to GenBank (Accession numbers in Table 1).
2.3. Molecular data analysis
Multiple alignments for both genes were made using ClustalW (Wang and Jiang, 1994).
Cladogramms were built by the neighbor-joining method (Saitou and Nei, 1987). Tree node
credibility values were calculated in 1000 iterations of the bootstrap analysis (Felsenstein, 1985).
COI sequences from NCBI GenBank (AF513645 – from the Northeast Pacific Ocean, Vancouver
Island; AF531750 – from the South Atlantic, Brantsfield Strait, 62.35 S, 58.54 W; AF474107 –
from the Southwest Pacific Ocean, off New Zealand; AF474106 – from the North Atlantic, Gulf
of Maine; AF259666 – from the North Atlantic, Georges Bank; AB380018– from the North
Pacific 40.01 N 145.01 E) were used along with the original data. Metridia gerlachei Giesbrecht,
1902 (AF531747 and AF536518) was used as an outgroup.
3. Hydrological features
Water temperature increased from the South to the North from -1.5 to +6ºС for the Drake
Passage and from -2 to +19ºС in the Eastern section during Antarctic spring, when samples were
collected. At the Eastern transect the isotherm +4ºС on depth 0-100m was located between the
Polar Front and the Subantarctic Front. In the Drake Passage the same isotherm at that period was
vertical and matched the Subantarctic Front. During Antarctic summer, at the Eastern section the
+4ºС isotherm at a depth of 100m matched the Polar Front and that at a depth of 300m matched
the Subantarctic Front. In the Drake Passage +4ºС isotherm at that period was vertical and
matched the Subantarctic Front.
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Mean temperatures (Table 2) show that the Drake Passage was colder at any given depth
of the 0-300m layer. In the Drake Passage temperatures above +4ºС were recorded only in the
Subantarctic Zone. In the Eastern cross-section such temperatures were found northward to the
Polar Front – in the Polar Frontal Zone, the Subantarctic Zone and the Subtropical Zone. This is
typical for the Antarctic Spring and Summer seasons.
4. Results
4.1. mtCOI gene polymorphism
A cladogram was generated by aligning partial sequences of COI mitochondrial gene
from 80 originally collected adult specimens of Metridia lucens and 6 partial sequences from
NCBI GenBank (Fig. 2A). Two clades of M. lucens were identified with 8% nucleotide
divergence with maximum divergence within the same clade being less than 1%.
Table 3 shows distribution of specimen from different locations among the clades. The
clade A contained all specimen from the Weddell Sea, all AZ samples from western and eastern
parts of Antarctic sector of the Southern Ocean, all specimen from PFZ of the Drake Passage and
several specimen from PFZ of the Eastern transect, one individual from SAZ of the Drake
Passage, and one individuals from the Bellingshausen Sea. The clade B contained all individuals
from STZ and SAZ, and several specimen from FPZ of the Eastern transect and one individual
from South-West Pacific (South off New Zealand).
The specimens from the Northern Hemisphere are close to the clade B. The divergence is
4% for the Northern Atlantic and 2% for the Northern Pacific.
4.2. ITS region polymorphism
A total of 82 individuals of the M. lucens complex were analysed based on ITS1-5,8S-
ITS2 region of nuclear DNA. Phylogenetic analysis of this dataset produced clades C and D with
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1% divergence (Fig. 2B). ITS1 has four highly variable positions and one slightly variable
position for 215bp and ITS2. It has one highly variable position and two slightly variable
positions for 180bp.
Table 3 shows the distribution of the specimen from different locations among the clades.
Copepods of the “C” clade form a single haplotype block (Table 4). Samples grouped to the “D”
(49 specimens) clade show an extent of the polymorphism in ITS1-5,8S-ITS2 region. This group
includes 8 samples from STZ, 10 from SAZ of the Eastern cross-section, 8 from SAZ of the
Drake Passage and 6 samples from PFZ of the Eastern cross-section.
Table 4 shows the states of 5 variable positions of ITS1 and 3 of ITS2. A considerable
amount of heterozygous states was detected, with maximum seven heterozygous positions in
individual D87 from STZ.
Clades C and D based on the ITS region match clades A and B in a mtCOI-based
cladogram.
5. Discussion
5.1. Taxonomic status
According to recent studies on mtCOI polymorphism for crustaceans (Waugh, 2007;
Costa et al., 2007, Radulovici et al., 2010) the boundary between closely related species is
accepted as 2,7 − 3%. Though, obviously, further studies are needed to clarify the status of the
two groups, the detected substitution level of 8% for mtCOI suggests the presence of two cryptic
species within the M. lucens complex.
Our comparative analysis of fragments of mitochondrial and nuclear DNA has shown that
all individuals with the ITS haplotype СТТСАСТТ belong to the mitochondrial clade A (Table
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4). No exceptions were found, even at those sites where both clades were present (e.g., PFZ of
the Eastern section). Thus, in the areas of coexistence we find no evidence for hybridization.
These two clades may correspond to reproductively isolated species. Analysis of polymorphism
in ITS1 and ITS2 regions reveals (Table 4) that MLS shows no sequence variations and is
homozygous for both ITS regions. MLN has nine polymorphic positions in these regions.
It should be noted that two individuals with high number of heterozygous positions in
ITS1 and ITS2 regions, D87 and D90, could be hybrids between MLN and MLS. However, they
were collected away from the zone where the two forms coexist. We conventionally name the
form represented in the clades A and C MLS (Metridia lucens South), and the form of the clades
B and D is named MLN (Metridia lucens North). Therefore, our results suggest that MLS is
the sister species to MLN, and manifest very low genetic variation, possibly due to younger age,
for smaller population sizes or repeated bottlenecks in more severe high-latitude environment.
Our data indicates the possibility of weak unidirectional gene flow towards North, suggesting that
MLS males may hybridize with MLN females. This conclusion is based on our finding of 4
specimen North from species boundaries with MLN mtDNA and heterozygous in few ITS sites,
which differentiate MLN and MLS.
Metridia lucens from the North Sea is considered as M. lucens s.s. as the species was
described originally near the Norway coast (Boeck, 1865). It is clear from Fig. 2 that both MLN
and MLS are genetically distinctive from M. lucens from the North Sea and cannot be considered
as M. lucens s.s. Currently M. lucens is considered to be widely distributed species with a wide
range of variability in morphology (Bradford-Grieve, 1999). There is a high possibility that
several closely related species were reported under the name M. lucens Boeck, 1865. To
determine and define the species inside the M. lucens complex it is crucial to re-describe M.
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lucens s.s. from the locality type based on extensive freshly collected material with involvement
of molecular and morphology analysis. Only upon the ranges of morphological variability of M.
lucens s.s. are determined it would be possible to describe new species in the M. lucens complex.
5.2. Spatial distribution of MLN and MLS and effects of the environment
The Southern Ocean is characterized by a complex system of water circulation (Belkin,
1993; Sokolov and Rintoul, 2009) dominated by the Antarctic Circumpolar Current (ACC). The
ACC can be divided into three main streams: Polar Front, Subantarctic Front, and Southern Front
(Orsi et al., 1995). Two major mechanisms of water exchange between interfrontal zones within
the ACC are known (Koshlyakov and Sazhina, 1996): surface or subsurface drift currents
(usually directed northward) and transfrontal exchange via gyres.
The habitat of MLN and MLS in the Southern Ocean is shown Fig. 3. MLS inhabits the
Polar Frontal Zone and the Antarctic Zone. An individual from the Bellingshausen Sea also
belongs to MLS. The MLN form inhabits the Subtropic Zone, the Subantarctic Zone and the
Polar Frontal Zone. An individual from South-West Pacific off New Zealand also belongs to
MLN. It is remarkable that the MLN population of the Southern Ocean is genetically close to M.
lucens s.s. of the Northern Hemisphere with 2% divergence for Northern Atlantic and 4% for
Northern Pacific in COI. This indicates that M. lucens s.s. from the Northern Hemisphere and
MLN are similar; MLN appears to be more abundant and more widely distributed than MLS.
In the Eastern section, MLN occurs North of the Polar Front and does not depend in its
distribution on other fronts. Conversely, in the Drake Passage, MLN occurs north of the Subpolar
Front. MLS depends in distribution on the Subantarctic Front on both sides of the Southern
Atlantic and does not depend on other fronts.
We suggest that the ranges of optimal temperature for survival and reproduction of MLN
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and MLS species are different, though overlapping. MLS was found at temperatures between -
2oС and +10
oС, while MLN was recorded between +4
oС and +12
oС (Fig. 4, 5). Thus, both were
detected at temperatures from +4 o
С to +10 o
С. Southward of the Polar Front MLN seems to be
represented by a few individuals. Most probably, MLN, on the contrary to MLS, can not
reproduce in water colder than +4 o
С, and the +4 o
С isotherm can be considered the southern
border of MLN population.
The fronts in the Drake Passage are shifted southward (Sokolov and Rintoul, 2009;
Sprintall, 2003, 2008). Therefore, water temperature of same hydrological zones is lower for the
Drake Passage than for the Eastern section (Table 2). The +4 o
С isotherm in the Drake Passage
matches the Subantarctic Front, but for the Eastern section it lies within the Polar Frontal Zone.
However, in both regions the +4 o
С isotherm matches MLN distribution border during both
spring and summer of the Southern Hemisphere.
In the Drake Passage, the individuals of the M. lucens complex are apparently transferred
through the Subantarctic Front only northward. The transfrontal water exchange in the Drake
Passage is known to be generally directed southward (Koshlyakov and Sazhina, 1996; Golivets
and Koshlyakov, 2004, 2009). However, M. lucens penetrates through the Subantarctic Front in
the opposite direction that may prove ecological nature of barriers: most likely both species of the
M. lucens complex are advected through the Subantarctic Front in both distections but MLN can
not survive and/or reproduce in colder waters south of the Polar Front. Between the Polar Front
and the Subantarctic Front both species co-occur in the same geographic locations. However,
they may be isolated vertically living at different depths in different water masses (Fig. 4, 5).
As it was shown by Stupnikova et al. (2013) Antarctic (South of PF) and Subantarctic
(North of PF) populations of two dominant zooplankters Rhincalanus gigas Brady, 1883 and
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Calanus simillimus Giesbrecht, 1902 (Copepoda: Calanoida) do not show any genetic difference.
Apparently the Polar Front can not represent an unpenetrable barrier for MLS and MLN, due to
active water exchange. Most likely, some ecological factors limit MLS and MLN spatial
distribution, while the effect of frontal zones seems to be indirect. In spite of current co-existence
of MLN and MLS in the Polar Frontal Zone, we cannot exclude significance of this isolation in
the past that let these two cryptic forms of copepods concur an ecological divergence via different
temperature tolerance. If so, the spatial coexistence in these two genetically isolated forms can
be a consequence of hydrological history in this area.
5.3. Cryptic species in marine zooplankton
Existence of cryptic species in marine plankton was suggested rather long ago (Knowlton,
1993). However, the mechanisms involved in speciation are appeared to be species-specific.
Some zooplankters show no considerable genetic difference for populations separated by
distances of about 1000 km: e.g. copepods Calanus finmarchicus (Bucklin and Kocher, 1996;
Bucklin et al., 2000), Nannocalanus minor (Bucklin et al., 1996), Pseudocalanus
acuspes (Holmborn et al., 2011), Calanus simillimus and Rhincalanus gigas (Stupnikova et al.,
2013); and also euphausiids Meganyctiphanes norvegica (Bucklin et al., 1997), Euphausia
superba (Zane et al., 1998; Zane and Patarnello, 2000), Euphausia crystallorophias (Jarman et
al., 2002).
On the other hand, many other species are represented by genetically distinct groups,
often recorded even within the same ocean water masses. In addition to the M. lucens complex
studied in this work, there are examples of other cosmopolitan species: the chaetognath
Eukrohnia hamata (Kulagin et al., 2012), the copepods Pleuromamma xiphias (Goetze, 2011)
and Eucalanus hyalinus (Goetze, 2005).
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Our data also demonstrates that the geographic distance is not critical for the plankton
isolation. The individuals of the M. lucens from the North Sea and the Subantarctic waters were
genetically more close than two groups found in the same area of the Polar Front Zone (Fig. 2).
Acknowledgements
This study was supported by the Russian Foundation for Basic Research (grant 12-05-
31383) and the Ministry of Education and Science of the Russian Federation (grant
11.G34.31.0008, grant 8132, grant 8057).
The authors are grateful to M. Flint, A. Vereshchaka, A. Pasternak (P.P. Sirshov Institute
of Oceanology RAS), A. Azovsky (Lomonosov Moscow State University), A. Kondrashov
(University of Michigan) and three anonymous referees for critical reading of the manuscript and
helpful comments. The authors thank K. Goupalo for helping in English language. We thank the
crew of the R/Vs «Akademik Ioffe» and «Akademik Sergey Vavilov» for assistance in sample
collection. We also greatly acknowledge kind help of A. Lunina, D. Kulagin, V. Gagarin in
collecting and sorting the samples. We thank E. Gorokhova (the Norwegian National Mesocosm
Centre, Espegrend, Universitetet in Bergen, Norway) who kindly provided the North Sea
specimen.
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Fig. 1 Sampling sites and ACC front configuration during sampling. A) 30th
Cruise of R/V
«Akademik Ioffe» B) 31th
Cruise of R/V "Akademik Sergey Vavilov". STF – the Subtropical
Front, SAF – the Subantarctic Front, PF – the Polar Front, SACCF – the Southern ACC Front.
STZ – the Subtropical Zone, SAZ – the Subantarctic Zone, PFZ – the Polar Front Zone, AZ – the
Antarctic Zone.
Fig. 2 Phylogeny of M. lucens based on partial sequences of mtCOI gene (A) and rDNA ITS1-
5.8S -ITS2 region (B) with Metridia gerlachei as an outgroup. Dr – the Drake Passage, E –
Eastern section. STZ – the Subtropical Zone, SAZ – the Subantarctic Zone, PFZ – the Polar Front
Zone, AZ – the Antarctic Zone, WS – the Weddell Sea, SW Pacific – South-West Pacific, N
Pacific – North Pacific, NW Atlantic – North-West Atlantic, Ant Peninsula – Antarctic
Peninsula, Bransfield Strait.
Fig. 3 Distribution of MLN and NLS species in the Southern Ocean. Front position by Orsi et al.,
1995. For abbreviations see Fig. 1.
Fig. 4 Geographical distribution of the species MLN (I) and MLS (II) at the Eastern section (А)
during Antarctic summer (December 2009) and (B) Antarctic spring (October 2010). For
abbreviations see Fig. 1.
Fig. 5 Geographical distribution of the species MLN (I) and MLS (II) at the Drake Passage (А)
during Antarctic summer (December 2009) and (B) Antarctic spring (October 2010). For
abbreviations see Fig. 1. PF 1, PF 2, PF 3 – the Southern Polar Current.
(A) (B)
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Table 1
Samples used. Location in different ACC hydrological zones: the Subantarctic Zone (SAZ), the
Polar Frontal Zone (PFZ), the Antarctic Zone (AZ), and the Subtropical Zone (STZ). NS – the
North Sea
Cru
ise
Dat
a
Zone
Sit
e
Longit
ude
Lat
itude
Lay
er
Vouch
er
GenBank
accession
number
mtCO1
GenBank
accession
number
rDNA
Drake Passage
R/V ASV-31 10.11.2010 SAZ 2276 -65,08 -57,21 0-300 F14
F15
D35
D36
JQ889929
JQ889930
JQ889884
JQ889885
JQ944760
JQ944718
JQ944778
JQ944776
R/V ASV-31 10.11.2010 SAZ 2281 -66,10 -56,66 0-300 F12
F13
D30
D31
JQ889927
JQ889928
JQ889867J
Q889883
JQ944720
JQ944719
JQ944779
R/V ASV-31 11.11.2010 SAZ 2283 -66,49 -56,57 0-300 F05
F6
JQ889921
JQ889922
JQ944716
JQ944715
R/V ASV-31 09.11.2010 PFZ 2271 -64,30 -57,94 0-300 D71
D72
D73
JQ889892
JQ889893
JQ944763
JQ944792
JQ944761
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D74
D75
D76
D77
D78
D79
D80
D81
D82
D83
D84
D85
JQ889894
JQ889895
JQ889896
JQ889897
JQ889898
JQ889899
JQ889900
JQ889901
JQ889902
JQ889903
JQ889904
JQ889905
JQ944768
JQ944788
JQ944762
JQ944767
JQ944791
JQ944764
JQ944733
JQ944765
JQ944769
JQ944770
JQ944793
JQ944774
R/V AI-30 03.01.2010 AZ 2296 -63,97 -61,82 0-300 A10
A22
JN588593
JN588595
JQ944759
JQ944757
R/V AI-30 04.01.2010 AZ 2300 -64,21 -61,17 0-300 A36 JN588598 JQ944754
R/V ASV-31 04.11.2010 AZ 2244 -60,02 -61,69 0-300 D59 JQ889887
R/V ASV-31 04.11.2010 AZ 2246 -60,27 -61,49 0-300 D44 JQ889886 JQ944790
R/V ASV-31 05.11.2010 AZ 2248 -60,55 -61,26 0-300 C23 JQ889874 JQ944783
R/V ASV-31 05.11.2010 AZ 2250 -60,89 -60,98 0-300 F09
F10
JQ889925
JQ889926
JQ944712
JQ944721
R/V ASV-31 06.11.2010 AZ 2258 -62,23 -59,81 0-300 F7
F8
JQ889923
JQ889924
JQ944714
JQ944713
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the Eastern section
R/V ASV-31 08.10.2010 STZ 2176 12,75 -37,13 0-300 D86
D87
D88
D89
D90
D20
D21
D22
D67
D70
JQ889906
JQ889907
JQ889908
JQ889909
JQ889910
JQ889877
JQ889878
JQ889879
JQ889888
JQ889891
JQ944777
JQ944732
JQ944731
JQ944730
JQ944728
JQ944738
JQ944781
JQ944772
JQ944766
R/V AI-30 12.12.2009 SAZ 2240 7,33 -44,43 0-300 A09
A87
A88
A89
JN588604
JN588605
JN588606
JQ944746
JQ944748
JQ944747
JQ944789
R/V ASV-31 12.10.2010 SAZ 2186 10,73 -40,07 0-300 D9 JQ944729
R/V ASV-31 13.10.2010 SAZ 2192 9,42 -41,82 0-300 F16
F17
JQ889931
JQ889932
JQ944775
R/V ASV-31 13.10.2010 SAZ 2192 9,42 -41,82 300-
1000
C18
C19
JQ889870
JQ889871
JQ944744
JQ944743
R/V ASV-31 14.10.2010 SAZ 2195 8,74 -42,69 0-300 F3
C20
JQ889919
JQ889872
JQ944742
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R/V ASV-31 15.10.2010 SAZ 2199 7,79 -43,84 0-300 C92
C93
F04
JQ889920
JQ944740
JQ944782
R/V AI-30 13.12.2009 PFZ 2242 6,81 -44,98 0-300 A32
A33
A82
A83
A84
A85
A86
JN588596
JN588597
JN588599
JN588600
JN588601
JN588602
JN588603
JQ944756
JQ944755
JQ944753
JQ944752
JQ944751
JQ944750
JQ944749
R/V ASV-31 17.10.2010 PFZ 2210 4,97 -46,95 0-300 D24 JQ889880 JQ944737
R/V ASV-31 17.10.2010 PFZ 2210 4,97 -46,95 300-
1000
D25
D26
JQ889881
JQ889882
JQ944736
JQ944780
R/V AI-30 20.12.2009 AZ 2273 0,00 -53,92 0-300 B81
B82
JQ889869 JQ944785
JQ944786
R/V AI-30 21.12.2009 AZ 2277 0,00 -55,24 0-300 A11
B63
JN588594
JQ889868
JQ944758
JQ944787
R/V ASV-31 21.10.2010 AZ 2224 0,82 -50,76 0-300 D04 JQ889875 JQ944735
R/V ASV-31 21.10.2010 AZ 2225 0,49 -51,02 0-300 C22
C82
JQ889873
JQ944741
R/V ASV-31 22.10.2010 AZ 2229 0,00 -52,28 0-300 C21
D96
JQ889913
JQ944784
JQ944726
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D97
D98
D99
F1
F2
JQ889914
JQ889915
JQ889916
JQ889917
JQ889918
JQ944725
JQ944724
JQ944723
JQ944722
JQ944717
R/V ASV-31 23.10.2010 AZ 2235 0,00 -54,25 0-300 D8
D68
D69
JQ889876
JQ889889
JQ889890
JQ944734
JQ944773
JQ944771
R/V AI-30 22.12.2009 AZ 2281 0,00 -56,56 0-300 B88 JQ944745
R/V ASV-31 24.10.2010 AZ 2240 0,00 -55,67 0-300 D91
D92
D15
JQ889911
JQ889912
JQ944727
JQ944739
18.05.2012 NS 60,40
-5,31 0 F80
F81
F82
F84
KC412248
KC412249
KC412250
KC414886
KC414887
KC414888
KC414889
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Table 2
The mean temperature for each hydrological zone (ºС) at a depth of 0/100/200 meters, as
measured at sampling locations
Drake Passage the Eastern section
R/V ASV-31
spring
R/V AI-30
summer
R/V ASV-31
spring
R/V AI-30
summer
Subtropical Zone 15.0/14.3/13.1 17.0/16.4/16.0
Subantarctic Zone 5.1/4.8/4.6 6.3/6.2/6.0 8.6/8.3/8.0 11.0/10.1/8.3
Polar Frontal Zone 3.1/2.1/1.8 3.3/2.7/2.4 4.2/4.2/3.8 6.0/5.0/3.4
Antarctic Zone 0/-0.8/1 1.1/-0.3/0.5 0.9/0.7/1.2 1.8/0.3/1.1
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Table 3
Distribution of samples from different hydrological zones among clades of cladogram from Fig.2
СО1 rDNA ITS1-5,8S-ITS2
Clade A Clade B Clade C Clade D
Without
clade
Drake Passage
Subantarctic Zone 1 9 1 6 2
Polar Frontal Zone 14 15
Antarctic Zone 10 9
African section
Subtropical Zone 10 7 2
Subantarctic Zone 10 1 10
Polar Frontal Zone 4 6 4 6
Antarctic Zone 16 19
Brantsfield Strait 1
South-West Pacific 1
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Table 4
Variable positions of ITS1-5,8S-ITS2 region state for individual samples
Vouch
er Zone
Secti
on
ITS1 ITS2 Clade
mtCO1 59 68 76 123 125 135 411 442 494
A33 PFZ E C T A C G C C T T B
A82 PFZ E . . . Y . . . . . B
A83 PFZ E Y . . Y . . . . . B
A84 PFZ E Y . . Y . . . . . B
D24 PFZ E Y . . Y . . . . . B
D25 PFZ E Y . . Y . . . . . B
D31 SAZ Dr Y . . Y . . . . . B
D36 SAZ Dr Y . . Y . . . . . B
F05 SAZ Dr T . . T . . . . . B
F06 SAZ Dr T . . T . . . W . B
F12 SAZ Dr Y . . Y R . . . W B
F13 SAZ Dr . Y . . R . Y . W B
F14 SAZ Dr T . . Y . . . . . B
F15 SAZ Dr Y . . Y . . . . . B
A87 SAZ E Y . . Y . . . . . B
A88 SAZ E Y . . Y . . . . . B
A89 SAZ E Y . . T . . . - - B
C18 SAZ E Y . . . . . . . . B
C19 SAZ E T . . T . . . . . B
C20 SAZ E Y . . . . . . . . B
F16 SAZ E T . . T . . . . . B
C92 SAZ E T . . T . . . . .
C93 SAZ E T . . T . . . . .
A09 SAZ E Y . . Y . . . . .
D67 STZ E Y . . Y . . . . .
D20 STZ E Y . . Y . . . . . B
D21 STZ E Y . . Y . . . . . B
D70 STZ E Y . . Y . . . . . B
D86 STZ E T . . T . . . . . B
D87 STZ E Y Y W Y R . Y . W B
D88 STZ E Y . . . . . . . T B
D89 STZ E Y . . . . . . . T B
D90 STZ E Y Y . Y R . Y . W B
D92 AZ E . . T . A . . . A A
D15 AZ E . . T . A . . . A
B88 AZ E . . T . A . . . A
A10 AZ Dr . . T . A . . . A A
A22 AZ Dr . . T . A . . . A A
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A36 AZ Dr . . T . A . . . A A
C23 AZ Dr . . T . A . . . A A
D44 AZ Dr . . T . A . . . A A
F07 AZ Dr . . T . A . . . A A
F08 AZ Dr . . T . A . . . A A
F09 AZ Dr . . T . A . . . A A
F10 AZ Dr . . T . A . . . A A
A11 AZ E . . T . A . . . A A
B81 AZ E . . T . A . . . A A
D04 AZ E . . T . A . . . A A
D08 AZ E . . T . A . . . A A
D68 AZ E . . T . A . . . A A
D69 AZ E . . T . A . . . A A
D96 AZ E . . T . A . . . A A
D97 AZ E . . T . A . . . A A
D98 AZ E . . T . A . . . A A
D99 AZ E . . T . A . . . A A
F01 AZ E . . T . A . . . A A
F02 AZ E . . T . A . . . A A
B63 AZ E . . T . A . . . A
B82 AZ E . . T . A . . . A
C21 AZ E . . T . A . . . A
C82 AZ E . . T . A . . . A
D72 PFZ Dr . . T . A . . . A
D71 PFZ Dr . . T . A . . . A A
D73 PFZ Dr . . T . A . . . A A
D74 PFZ Dr . . T . A . . . A A
D75 PFZ Dr . . T . A . . . A A
D76 PFZ Dr . . T . A . . . A A
D77 PFZ Dr . . T . A . . . A A
D78 PFZ Dr . . T . A . . . A A
D79 PFZ Dr . . T . A . . . A A
D80 PFZ Dr . . T . A . . . A A
D81 PFZ Dr . . T . A . . . A A
D82 PFZ Dr . . T . A . . . A A
D83 PFZ Dr . . T . A . . . A A
D84 PFZ Dr . . T . A . . . A A
D85 PFZ Dr . . T . A . . . A A
A32 PFZ E . . T . A . . . A A
A85 PFZ E . . T . A . . . A A
A86 PFZ E . . T . A . . . A A
D26 PFZ E . . T . A . . . A A
D35 SAZ Dr . . T . A . . . A A
D09 SAZ E . . T . A . . . A
F84 North Sea . W Y R Y . . W
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F81 North Sea . W Y R Y . . W F80 North Sea . T . A T . . A F82 North Sea . W Y R Y . . A
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Highlights
The study is based on materials collected in the Atlantic part of the Southern Ocean where the
water masses structure and oceanographic fronts over isolation of populations of abundant
zooplankton species.
These two groups were considered as representing two cryptic species within M. lucens: M.
lucens North and M. lucens South. These forms are found mainly to the north and to the south of
the South Polar Front. No hybrids between the two forms were detected.
We propose that the temperature is the limiting factor for M. lucens North, which inhabits the
waters warmer than 4°C. The frontal zones seem to have no direct effect on distribution.