Universidade de Lisboa
Faculdade de Ciências
Departamento de Biologia Animal
“Cephalopod Fauna in the Southern Ocean using the diet of wandering albatrosses Diomedea exulans : a stable isotopes approach”
Miguel Fernandes Guerreiro
Dissertação
Mestrado em Ecologia Marinha
2012 Universidade de Lisboa
Faculdade de Ciências
Departamento de Biologia Animal
“Cephalopod Fauna in the Southern Ocean using the diet of wandering albatrosses Diomedea exulans : a stable isotopes approach”
Miguel Fernandes Guerreiro
Dissertação Orientada pelo Prof. Doutor Rui Rosa da Faculdade de Ciências da Universidade de Lisboa e Doutor José Xavier do Instituto do Mar em Coimbra e do British Antarctic Survey
Mestrado em Ecologia Marinha
2012
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Á memória de Josefa Esteves Afonso (17/03/1933 23/09/2011),
carinhosamente chamada por avó.
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AGRADECIMENTOS
Quero agradecer ao meu orientador externo Dr. José Xavier pela oportunidade em fazer uma tese desta escala, e focada na Antártida. Foi um excelente orientador, já que me guio em todo o processo do desenvolvimento de uma dissertação cientifica e todo o processo por detrás desta, e levou me aos melhores locais da Europa (e senão do Mundo) para se fazer ciência Polar e apresentou me os maiores especialistas na matéria. Para rematar, e citando o mesmo, foi um orientador “Brutal” (Xavier, 2007).
Ao meu orientador interno Dr. Rui Rosa, que puxou por mim, e me “puxou pelas orelhas” quando foi preciso.
Ao Dr. Yves Cherel, pelos seus comentários, perspectivas e conhecimentos que me passou fundamentais para a minha dissertação.
Ao Dr. Filipe Ceia, pela sua paciência e compreensão no laboratório de Coimbra (IMAR). Se não fosse ele, provávelmente os meus resultados estariam todos contaminados devido á minha inexperiência.
Á Dr. Alexandra e á Dr. Gabriela (IMAR), por correr as análises de isótopos estáveis e “tomar contar” da minha equipa de trabalho respectivamente.
Á minha equipa de trabalho (Pedro Alvito e José Seco), pela a ajuda no processamento de mandíbulas de cefalópodes em Coimbra.
Á minha irmã pela ajuda na formatação do texto da tese.
Á minha Familia, e ao meu grupo de amigos, ambos por me ouvirem um bilião de vezes a falar de isótopos, e responderem me de volta, e claro, pela afeição que nutrem por mim.
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ABSTRACT
The Southern Ocean is a key component in the climatic and ecological global system. Cephalopods play an important task in this ecosystem. However, they are difficult to collect and therefore the basic knowledge regarding their ecology is scarce. The wandering albatross, Diomedea exulans , is a cephalopod predator. Here I characterize the cephalopod component of D. exulans diet by collecting boluses and regurgitates of chicks from around the ocean, in South Georgia, Crozet and Kerguelen Islands. By using stable isotopes analyses of Nitrogen and Carbon on the squids found on the diet, I can determine the distribution and trophic level of them, an approach that may provide important information about the threats of D. exulans .
D. exulans fed predominantly in Onychoteuthid and Histioteuthid squids and secondarily on cranchiids and giant squids. Kerguelen diet differs from the others due to the influence of these large bodied squids, further proving the idea that much of the diet of these seabirds comes from scavenging.
Cephalopods of the Southern Ocean were distributed within three water masses (Subtropical, Subantarctic and Antarctic), except for South Georgia (Antarctic and Subantarctic). Much of the previous biogeographic distributions of these squids in the Indian sector were confirmed or expanded north, for the subantarctic region. Cephalopods on the Southern Ocean occupy a great trophic span, from Martialia hyadesi (3.52±0.25 TL) to Taningia danae (6.01±0.15 TL).Thus, squids play a key role in the trophic ecology of D. exulans , that feeds mainly of Antarctic and Subantarctic and secondarily of Subtropical squids.
Based on these findings, we may argue that D. exulans have different threats within the Southern Ocean: in the Atlantic, Longliners operating in the nearby shelves are the main threat; In the Indian sector, there is different contributions from Subtropical Tuna fishing and longliners in the shelves, at the two studied islands.
Key-Words: Cephalopods, Southern Ocean, Stable Isotopes, Diomedea exulans .
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RESUMO
O Oceano Antártico, também conhecido como Oceano Austral e Oceano Glacial Antártico, é constituído por uma série de bacias abissais oceânicas, interrompidas pelas cristas oceânicas de Scotia e Macquarie e pela plataforma continental de Kerguelen.
Este oceano representa um importante componente tanto do Clima e Oceano global, como também da Bioesfera. É aqui que se inicia a corrente termohalina profunda, fundamental para a vida submarina planetária devido ao abastecimento de oxigénio às camadas mais profundas do oceano, e para a vida à superfície, visto que transporta nutrientes das profundezas para os produtores primários pelágicos. Também é nesta região que se encontra a corrente circumpolar antártica, acompanhada pelas vagas e ventos de oeste que aumentam a profundidade da camada homogénea superficial (conceito fundamental em produção primária). Para a existência destes fenómenos fundamentais e para a manutenção da calote glacial é essencial que as temperaturas registadas na Antártida permaneçam abaixo de zero.
Deste Oceano dependem vários animais para se reproduzirem e alimentarem, nomeadamente a ave com maior envergadura de asas do nosso planeta, o Albatroz Errante ( Diomedea exulans ). Esta espécie está, segundo a União Internacional para a Conservação da Natureza (I.U.C.N), vulnerável à extinção, em muito devido à mortalidade que advém da interação desta ave com barcos de pesca que operam nas suas áreas de alimentação. Os aparelhos atualmente utilizados para seguir estes animais quando partem para o mar em busca de alimento apenas nos fornecem dados de localização e massa do alimento, mas nada acerca de intensidade ou frequência de itens ingeridos, nem a categoria taxonómica a que esses itens pertencem.
Uma dessas categorias taxonómicas, a teutofauna, é composta pelos cefalópodes (lulas e polvos), que, no oceano Austral apresentam um alto grau de endemismo, e muitas divisões taxonómicas não se encontram aqui presentes, como é o caso dos chocos e lulas Myopsidas. Teoriza se que a teutofauna seja responsável por uma cadeia trófica alternativa ao Krill ( Euphausia superba ) e que substitua o nicho alimentar dos grandes peixes epipelágicos. Estes moluscos são muito esquivos, conseguindo evadir se muito eficazmente à captura por métodos tradicionais tanto pelos cruzeiros científicos, como por barcos de pesca, daí a informação atualmente disponível relativamente a estes animais nesta região ser reduzida.
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Nos últimos anos têm sido desenvolvidas técnicas e metodologias com isótopos estáveis de Carbono e Azoto que pemitem averiguar a partir das assinaturas destes elementos (razão entre a concentração do isótopo mais pesado sobre a do mais leve) nas mandibulas inferiores das lulas, a distribuição latitudinal e posição trófica (respetivamente) destes animais. A assinatura de Carbono é caracteristico de cada latitude neste Oceano, logo informa onde as lulas se alimentaram, e como a assinatura de Azoto enriquece de uma forma mais ou menos linear de nível trófico em nível trófico, é possivel calcular níveis tróficos com esta assinatura.
Assim, este estudo pretende averiguar a intensidade de captura de cefalópodes pelo D. exulans ao longo do oceano em estudo, através da caracterização da dieta em cefalópodes deste e averiguar a distribuição geográfica (e trófica) destes cefalópodes, e finalmente, inferir a partir desta informação consequências conservacionistas para o D. exulans .
Para tal, obtiveram se regurgitações induzidas e boluses de crias de D. exulans nas ilhas da Geórgia do sul, Crozet e Kerguelen, donde se recolheram as mandíbulas dos cefalópodes usadas neste estudo. Através da identificação de cada mandíbula e uso de equações alométricas para estrapolar o peso da lula a partir do tamanho da mandíbula, foi possível obter valores da abundância numérica e em massa das várias espécies, e assim caracterizar a dieta.
Para averiguar a distribuição latitudinal das lulas, foram consideradas as assinaturas de Carbono superiores a 19,5‰ e inferiores a 22,3‰ como subtropicais e antárticas, respetivamente, e as que se encontravam entre estes limites, como subantárticas. Enquanto que para o cálculo do nível trófico, foi usada uma função linear que transforma a assinatura de Azoto da mandíbula em nível trófico.
Com os dados obtidos nas alíneas anteriores, foi possível obter a latitude média em que os cefalópodes da dieta vivem, através do cálculo da média da assinatura de Carbono das lulas encontradas na dieta, ponderando a com o peso (neste caso a percentagem de indivíduos) que as espécies têm na dieta.
A dieta na Geórgia do sul e Crozet foi dominada em número pelas lulas Kondakovia longimana (24,2% e 33,7%), Taonius sp B (Voss) (23,7% na Geórgia do sul), Galiteuthis glacialis (8,8% em Crozet) e Histioteuthis eltaninae (10,6% e 25,3%).
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Em Kerguelen, a ordem de importância do contributo em número é o inverso da observada nas outras ilhas, com Histioteuthis atlantica (29,9%) a dominar, seguida por G. glacialis (12,2%) e finalmente K. longimana (10,0%).
Em todas as ilhas, K. longimana destacou se como a principal espécie a contribuir para a massa encontrada na dieta (75.5%, 76.0% e 31.0% na Geórgia da sul, Crozet e Kerguelen respetivamente), mas em Kerguelen verificou se que lulas gigantes ( Architeuthis dux e Taningia danae ) também contribuem com alguma importância para a massa total da dieta (15,0% e 13,2%). A espécie Histioteuthis atlantica , devido ao grande número de individuos encontrado em Kerguelen , acabou por ter um grande contributo por massa (12,9%).
As diferenças verificadas nas dietas sustentam que no setor atlântico deste Oceano, os albatrozes dependem mais de Taonius sp. B (Voss), Gonatus antarcticus e Mastigoteuthis sp. A (Clarke) que no setor Indico, pois neste último setor os albatrozes têm disponível uma maior variedade de lulas devido à proximidade aos subtrópicos. Foram verificados indícios de necrofagia, pois várias lulas encontradas pesavam várias vezes mais que um albatroz adulto (aproximadamente 45 Kg e 12 Kg respetivamente).
As lulas analisadas neste estudo apresentam distribuição desde a zona Subtropical á Antártica. As espécies identificadas como subtropicais foram a H. atlantica , Cycloteuthis akimushkini e Taonius sp. (Clarke), e como espécies antárticas foram identificadas a Batoteuthis skolops e Gonatus antarcticus . K. longimana e Moroteuthis knipovitchi também se encontraram em águas antárticas, mas em alguns locais da amostragem mostraram distribuição subantártica devido ao efeito que a proximidade à costa tem sobre a assinatura isotópica de Carbono, e também ao facto de já terem sido observadas a norte da frente polar antártica. Todas as espécies apresentaram a mesma distribuição que a previamente observada, exceto G. antarcticus que foi observada no Antártico e Galiteuthis glacialis com a Alluroteuthis antarcticus no subantártico perto da frente subtropical.
As lulas analisadas distribuem se por 3 níveis tróficos diferentes, desde o final do terceiro até ao início do sexto, com a Martialia hyadesi a representar o terceiro nível (alimentando se potencialmente de copépodes e krill), seguida no quarto pela K. longimana e Moroteuthis ingens (alimentando se potencialmente de mictófideos e outros peixes mesopelágicos). No início do quinto nível estavam presentes várias espécies que são características do meio mesopelágico
7 como H. eltaninae e Haliphron atlanticus e a meio deste nível encontra se B. skolops e M. sp. A (Clarke), duas espécies muito similares, e que provavelmente têm a mesma estratégia alimentar que outros Mastigoteuthideos, ou seja, alimentam se de zooplânton bentopelágico. Nos níveis tróficos mais elevados, encontra se G. antarcticus , T. sp. B (Voss) e Taningia danae , que se alimentam de presas com assinaturas de Azoto elevadas devido a encontrarem se em cadeias tróficas muito inefecientes ou a serem predadores de topo. Não foi possível a determinação de níveis tróficos na zona subtropical, mas C. akimushkini apresenta a assinatura de Azoto mais alta, e H. atlantica mais baixa. A espécie H. atlantica revela um crescimento da assinatura de Azoto com o aumento do tamanho do animal.
A média ponderada da assinatura de Carbono das dietas dos albatrozes em lulas e a assinatura de Carbono das principais lulas da dieta mostrou que na Georgia do sul os albatrozes se alimentam em média na zona da frente polar, limitando se mais a água subantárticas e proximas das plataformas continentais desta região, onde ocorre a pesca do Bacalhau da Patagónia (Dissostichus eleginoides ), enquanto que no setor indico, alimentam se mais a norte na zona subantártica, perto da plataforma continental das ilhas Kerguelen (onde opera a pesca ao D. eleginoides ), ou no mar aberto entre estas e as Crozet.
Em Kerguelen, se os dados da dieta estiverem certos acerca da importância da H. atlantica , estas aves alimentam se principalmente na zona subtropical onde ocorre a pesca ao atum Thunnus maccoyii e secundariamente na plataforma continental da ilha onde são residentes (onde opera a pesca ao D. eleginoides ), se H .atlantica afinal não for tão importante, a principal zona de alimentação será mesmo a plataforma continental, com os seus respetivos perigos.
Assim, K. longimana domina a dieta de D. exulans , com diferentes contribuições das outras familias de lulas nas várias ilhas. As lulas presentes na dieta vêm desde a zona subtropical até á Antártida com exceção na Geórgia do sul, onde não se registaram lulas dos subtrópicos. A importância na cadeia trófica destes animais foi confirmada, encontrando se animais de vários níveis tróficos. A principal ameaça ao D. exulans é a pesca dos palangreiros nas plataformas continentais desta região, e em Kerguelen, a pesca ao Atum Thunnus maccoyii .
Palavras-Chave: Cefalópodes, Antártico, Isótopos estáveis, Diomedea exulans.
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TABLE OF CONTENTS
1. Introduction ...... 15
1.1 Southern Ocean oceanography and climate...... 15
1.2 Southern Ocean cephalopods...... 17
1.3 Wandering albatrosses as a sampling predator of cephalopods ...... 18
1.4 Using stable isotopic signatures of cephalopods beaks ...... 19
1.5 Objectives ...... 20
2. Material and Methods...... 21
2.1 Study Area and sampling ...... 21
2.2 Characterization of cephalopod component in the albatross’ diet ...... 21
2.3 Stable isotopes analysis ...... 23
2.3.1 Isotope Modeling...... 24
2.4 Statistical Analyses ...... 24
3. Results ...... 26
3.1 Overall ...... 26
3.1.1 Diet ...... 26
3.1.2 Stable isotopes ...... 26
3.2 South Georgia ...... 27
3.2.1 Diet ...... 27
3.2.2 Stable isotopes ...... 33
3.3 Crozet ...... 36
3.3.1 Diet ...... 36
3.3.2 Stable Isotopes...... 37
3.4 Kerguelen...... 40
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3.4.1 Diet ...... 40
3.4.2 Stable Isotopes...... 41
3.5 Comparison between islands ...... 44
3.5.1 Diet indexes ...... 44
3.5.2 Diversity and cumulative curves ...... 44
3.5.3 Spatial differences of cephalopod species parameters and signatures ...... 46
3.5.4 Overall trophic level assessment ...... 49
3.5.5 Isotope modeling of wandering albatrosses foraging waters ...... 50
4. Discussion ...... 51
4.1 Methodological limitations ...... 51
4.2 Spatial differences in the cephalopod diet of wandering albatrosses ...... 53
4.3 Cephalopod habitats in the Southern Ocean and adjacent waters ...... 55
4.4 Cephalopod trophic position in the Southern Ocean and adjacent waters ...... 57
4.5 Implications on the conservation of wandering albatrosses ...... 60
5. Final considerations...... 62
6. Bibliography ...... 63
7. annexs ...... 71
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LIST OF FIGURES
Figure 1.1 The Southern Ocean. Emerged areas are green coloured. Parallels are spaced 10º and meridians 20º. The geographical position of the breeding islands of D.exulans South Georgia, Prince Edward, Crozet, Kerguelen, Heard & Macdonald and Macquarie on the Southern Ocean. The main surface water circulation in the Southern ocean is also represented (Orange arrows – warmer waters; Blue arrows – colder waters of the Circumpolar Current) with the 1000 m isobath. Main Oceanic fronts are present in the map on the left. Legend: PF Antarctic Polar Front; SAF Sub Antarctic Front; STF Sub Tropical Front. (Source: Orsi et al., 1995) ...... 15
Figure 3.1 Lower Rostral Length (LRL) distribution of the squids found on the diet of Wandering Albatross in South Georgia, Crozet and Kerguelen...... 26
Figure 3.2 – Lower Rostral Length (LRL) distribution of the squids found on the diet of Wandering Albatross in South Georgia...... 28
Figure 3.3 Distribution of the stable isotopes signatures of the squids of South Georgia. Top panel shows the Carbon signature(Red line and Blue line correspond to Subtropical and Polar fronts respectively from ( Cherel & Hobson, 2007)) and in the Bottom panel the Nitrogen signature. "L" and "S" in front of Histioteuthis atlantica stand for large and small specimens respectively...... 35
Figure 3.4 Lower Rostral Length (LRL) distribution of the squids found on the diet of Wandering Albatross in Crozet...... 36
Figure 3.5 Distribution of the stable isotopes signatures of the squids of Crozet. Top panel shows the Carbon signature (Red line and Blue line correspond to Subtropical and Polar fronts respectively from ( Cherel & Hobson, 2007)) and in the Bottom panel the Nitrogen signature. . 39
Figure 3.6 Lower Rostral Length (LRL) distribution of the squids found on the diet of Wandering Albatross in Kerguelen...... 40
Figure 3.7 Distribution of the stable isotopes signatures of the squids of Kerguelen. Top panel shows the Carbon signature (Red line and Blue line correspond to Subtropical and Polar fronts respectively from ( Cherel & Hobson, 2007)) and in the Bottom panel the Nitrogen signature. "L" and "S" in front of Histioteuthis atlantica stand for large and small specimens respectively...... 43
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Figure 3.8 Coleman Curves of the squid diversity in South Georgia, Crozet and Kerguelen. ... 45
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LIST OF TABLES
Table 3.1 Lower Rostral Length (LRL), Mantle Length (ML) and Weight (W) of the main species found on the diet of Wandering Albatrosses of South Georgia, Crozet islands and Kerguelen. (Continued next page) ...... 29
Table 3.2 Frequency of occurrence (F%), number of beaks (N%) and estimated mass(W%) of the main species contributing to the diet of Wandering Albatross in South Georgia, Crozet and Kerguelen. All species in Table 7.3 in annex...... 33
Table 3.3 Lower Rostral Length (LRL), Nitrogen and Carbon stable isotopes signatures of the main species found on the diet of Wandering Albatrosses of South Georgia...... 34
Table 3.4 Lower Rostral Length(LRL), Nitrogen and Carbon stable isotopes signatures of the main species found on the diet of Wandering Albatrosses of Crozet...... 38
Table 3.5 Lower Rostral Length(LRL), Nitrogen and Carbon stable isotopes signatures of the main species found on the diet of Wandering Albatrosses of Kerguelen...... 42
Table 3.7 Tests results of the Nitrogen stable isotopes signatures of the squid species analysed. Legend: A – Anova; T – T test; T(EXP) – T test, to exponentially transformed data...... 47
Table 3.8 Tests results of the Carbon stable isotopes signatures of the squid species analysed. Legend: A – Anova; T – T test...... 48
Table 3.9 Trophic level of the main Antarctic and Sub Antarctic species found on the diet of Wandering Albatrosses of South Georgia, Crozet and Kerguelen...... 49
Table 3.10 Mean Stable isotopes signatures of carbon and Nitrogen of the cephalopod component of the diet of Wandering Albatrosses of South Georgia, Crozet and Kerguelen...... 50
Table 7.1 – Alometric equations chosen from Xavier & Cherel (2009). Legend: a Chiroteuthid family formula; b Brachioteuthid family formula; c Cranchiid family formula; d Taonius spp. formula; e Gonatus spp. Formula; f Cycloteuthis akimushkini formulas; g Galiteuthis glacialis formula...... 72
Table 7.2 – Distribution of mantle length (ML), weight (W) and LRL from all squids found on D. exulans diet in the South Georgia, Crozet and Kerguelen islands...... 75
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Table 7.3 – All squid items found on the D. exulans diet throughout the three studied isands, and their respective contributions to the diet in terms of frequency, numeric and mass indexes...... 84
Table 7.4 – Chi squared results on the diet indexes (Frequency of occurrence (F%), numeric (N%) and mass (W%) indexes)...... 88
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1. INTRODUCTION
1.1 Southern Ocean oceanography and climate
The Southern ocean consists of a system of deep sea basins separated by the Scotia Ridge (South of the Falklands), the Kerguelen plateau (in the Indian section) and the Macquarie Ridge (South of New Zealand) (Carmack, 1990) and is limited in the South by the Antarctic continent (Figure 1.1).
Figure 1.1 - The Southern Ocean. Emerged areas are green coloured. Parallels are spaced 10º and meridians 20º. The geographical position of the breeding islands of D.exulans South Georgia, Prince Edward, Crozet, Kerguelen, Heard & Macdonald and Macquarie on the Southern Ocean. The main surface water circulation in the Southern ocean is also represented (Orange arrows – warmer waters; Blue arrows – colder waters of the Circumpolar Current) with the 1000 m isobath. Main Oceanic fronts are present in the map on the left. Legend: PF-Antarctic Polar Front; SAF- Sub-Antarctic Front; STF-Sub-Tropical Front. (Source: Orsi et al., 1995)
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The northern part is surrounded by the relatively warmer waters of the Antarctic Polar Frontal Zone (APFZ), beginning at the Antarctic convergence or Antarctic Polar Front (APF), which varies temporally and spatially between the 47ºS and 63ºS latitudes and it is characterized by a horizontal thermocline of 2 3ºC and other oceanic clines (Carmack, 1990; Orsi et al., 1995; Moore et al . 1997; Trathan et al . 1997; Moore et al., 1999). The main surface current is the Antartic Circumpolar Current (ACC) that runs eastwards around the continent.
Other important oceanic features in this ocean are the Sub Antarctic Front (SAF; it sets the end of the APFZ waters and the beginning of the Sub Antarctic waters), formed by the mixture of southern waters brought by the ACC and Northern tropical waters, and the Subtropical convergence or Subtropical Front (STF) (near the 40ºS latitude) (Deacon, 1982). The ACC with the APF, constitute a biological barrier, making this ocean virtually closed to all outside species (Collins & Rodhouse, 2006).
The fronts mentioned above are delineated by wind and oceanic features. Most of the Southern ocean is characterized by strong West winds, except for the area near the continent, where East winds predominate. The area of transition of this two wind regimes near the continent, it is called the Antarctic divergence, and it is characterized by low pressures and upwelling. The APF or Antarctic convergence, is the region where the Westerlies and Ekman drift are stronger (Deacon, 1982). The STF or Subtropical convergence occurs where the Westerlies meet the Trade winds, and the Antarctic waters sink to unusual depths, suggesting strong downwelling (Deacon, 1982).
Southern Ocean is a key component of the climate system in our planet. The deep thermo haline current (THC) starts in this region, fueled by a density shift in the waters due to the low temperatures, and increase in salinity due to the formation of oceanic ice (Sarmiento et al., 2004). Also, the low temperatures in this area (great thermal shift) in comparison to surrounding regions, allows the formation of strong winds, which maintain a strongly deep mixed layer on the surface of this ocean with high concentrations of nutrients.
This region is therefore, particularly sensitive to climate change as all of its currents and physical oceanographic and atmospheric processes are deeply dependent of below zero temperatures in the system, to fuel the THC and winds, and to maintain the Antarctic Ice Cap. The latter, if melted, would interrupt the THC, and increase global sea levels by approximately 60 meters (Church & Gregory, 2001 ).Thus, if any changes in the temperature of this ocean are verified in
16 the future, they will have great repercussions not only in this area and their inhabitants, as for the global ocean and planet.
Besides playing a key role in the replenishment of dissolved oxygen in the deep sea, this region also brings nutrients that are deposited in the sea bottom (or in deep waters) back to the surface (Sarmiento et al., 2004).
Last but not the least, the Southern Ocean is the habitat for numerous seabirds and marine mammal species, which depend on this ocean productivity and remoteness for foraging and breeding, respectively.
1.2 Southern Ocean cephalopods
Cephalopods play an important role in the marine food web of the Southern Ocean, since some of them occupy the niche of epipelagic top predators, normally occupied by sharks and large fish, and constitute part of an alternate food chain to krill (Rodhouse & White, 1995). These factors make cephalopods target of predation by many top marine predators (e.g. toothed whales, seals, penguins and Procellariform birds), and enable them to sustain large populations in the region (Xavier & Cherel, 2009). In fact, it has been estimated that top marine predators consume around 34 million tonnes of cephalopods per annum (Clarke, 1983).
Despite their important bio ecological role in the Southern ocean, the basic knowledge of the ecology of cephalopods is poorly known (Xavier et al., 1999). One of the main reasons for that is the fact that the Southern Ocean cephalopods have not awakened the interest of fishery industry, due to: i) the low number of exploitable species ii) the unpredictability of such stocks, iii) Lack of knowledge of the abundance and distribution of relevant species and iv) our inability to catch them ( Cherel et al., 2004; Collins & Rodhouse, 2006; Rodhouse 1998).
Also, the scientific cruises carried out in this area are unable to capture these animals due to the low speeds they practice, and as well for the orthodox sampling methods used (Rodhouse 1990, Rodhouse et al. 1996, Clarke 1977, Xavier et al., 2007).
It is worth noting that the cephalopod fauna of the Southern ocean deeply differs from the cephalopod fauna of the rest of the world. It consists of endemic species of octopods (cirrate and incirrate) and oegopsid squids, with a total absence of cuttlefish. Also myopsids are absent, and normally abundant families are rare or nonexistent. Only here we can find the Psychroteuthidae
17 and Batoteuthidae squid families, and the genera Mesonychoteuthis , Psychroteuthis , Kondakovia , Alluroteuthis , Slosarczykovia and Batoteuthis .
The oegopsid squids in this ocean are exclusively pelagic or benthopelagic and most have circum Antarctic patterns of distribution. The cephalopod fauna can be divided into species entirely Antarctic, and those that span the APF. These last ones either are migratory species or are deep sea animals, to which the APF has no biological meaning.
The main squid families found in this ocean are the: i) Onychoteuthids (e.g. including the Kondakovia and Moroteuthis genera), ii) Ommastrephids (mainly Martialia hyadesi ), iii) Gonatids (e.g. Gonatus antarcticus ), iv) Cranchids (including the colossal squid Mesonychoteuthis hamiltoni ), v) Neoteuthids (mainly Alluroteuthis antarcticus ), vi) Batoteuthids (with only Batoteuthis skolops ), vii) Mastigoteuthids (e.g. Mastigoteuthis psychrophila and M. sp. A (Clarke)), and viii) Histioteuthids.
1.3 Wandering albatrosses as a sampling predator of cephalopods
As an alternative to the more conventional methods used to study the biology of cephalopods from the Southern Ocean, a different approach has been recently applied, namely the use of seabird predators to sample cephalopods (Xavier et al . 2003a).
In this study, it was used the wandering albatross ( D. exulans ), the seabird with the largest wing span (with over 3 meters) that allows them to practice of long distance flights with low energetic requirements (Weimerskirch et al., 2000), for instance, during its annual circum antarctic migration. In general, albatrosses are an excellent tool for this kind of studies, because: i) they feed on a great amount and diversity of cephalopods (Rodhouse et al., 1987; Tickell 2000), ii) their populations gather around every year in high density colonies, iii) they do not fear the human presence, iv) cover large foraging areas to feed their chicks, which in turn v) maintain undigested parts of their prey in the stomachs for long periods of time (e.g. cephalopod statoliths and beaks).
D. exulans is thought to explore vast areas of the ocean seeking for large blotches of dying post spawning cephalopods that float up to the surface after death or near death (Lipinski & Jackson 1989),or for regurgitated stomach contents of sperm whales (Clarke et al., 1981). These assumptions are supported by the fact that their diet includes many deep sea cephalopods, i.e.,
18 animals that are usually found in depths out of the albatross reach (note: the maximum depth reach of the D. exulans is normally the length of its neck).
The main nesting colonies of D. exulans are found in islands and archipelagos of the sub/peri antarctic regions of South Georgia, Prince Edward, Crozet, Kerguelen and Macquarie (Figure 1.1). It is a biannual reproducing species, starting its mating season in the beginning of the austral summer (late November) and ending in the summer of the following year (December) (Tickell, 2000). By that time, the chicks regurgitate boluses with all the undigested parts of the meals that the parents gave to them up to that point, and leave the colony, for the first time, into the ocean.
During this period, breeding D. exulans make foraging trips to the surrounding ocean, which change in both length and time spent according to the state of development of the chick. Females go further North than males (Nel et al., 2002 ;Xavier et al., 2004), and it is by far, during incubation, that the parents perform the longest foraging trips. When chicks are born, parents limit their trips, becoming shorter and closer to the colonies continental platform (Weimerskirch et al., 1993; Nel et al., 2002).
According to the International Union for Conservation of Nature (IUCN), D.exulans is presently in a vulnerable state of conservation, due to several causes, one of them is due to being a by catch of the long liners operating in foraging areas (Gales 1993, Gales 1998, Prince et al., 98). The reason behind the common visits to these fishing vessels is the hope to get an easy meal. Although the foraging areas of wandering albatrosses are well known, the foraging effort in such areas has not been quantified yet, as the information of the devices used in foraging behavior studies can only give us the information about the feeding location and the mass of their food intake, with no taxonomic or categorical information.
1.4 Using stable isotopic signatures of cephalopods beaks
In the last couple of decades, stable isotopes analysis has been used to study trophic web ecology, namely by using the isotopes of Carbon (of atomic weights 12 and 13) and Nitrogen (of atomic weights 14 and 15), to gather information of geographic position and trophic level of biological samples, respectively (DeNiro & Epstein, 1978; DeNiro & Epstein, 1981).
19
The stable isotope signature of Carbon is influenced by limitations occurring during the photosynthesis of the autotrophs (the bottom of the food web), mainly by the activity of the
Rubisco or by the concentration of the substrate (CO 2) that limits the fixation of Carbon. This translates into an impoverishment or enrichment in heavy isotopes of Carbon 13, respectively. As the activity of Rubisco is gradually more limited in the upper latitudes of the ocean due to the decline of sea surface temperatures (SST) (Sackett et al., 1973), and at the same time, the increase in CO 2 available for the photosynthesis, a latitudinal gradient can be verified from the equator to the poles (Cherel & Hobson, 2007; Jaeger et al., 2010). This signature is then passed up throw the food chain with very low variability (DeNiro & Epstein, 1987).
The stable isotope signature of Nitrogen is useful to calculate the trophic level of a sample, as the heavier isotope of Nitrogen 15 accumulates from trophic level to trophic level in a linear way (Minagawa & Wada, 1984), and integrates the Nitrogen signatures of the different items of the diets.
Cherel & Hobson (2005) were the first to adapt and calibrate the stable isotopes methodology for the cephalopod beaks found on the diet of several of their predators, and by using the respective signatures, they confirmed the geographic position and trophic levels of reference species, and extrapolated to the rest of the species in that study. The present study intends to apply this methodology to the beaks found on the: i) boluses regurgitated by the wanderers’ chicks and ii) induced regurgitations of the chicks after being feed by their parents.
1.5 Objectives
Under this content, the main objectives of this study are to:
• Characterize the cephalopod diet of wandering albatrosses from the Atlantic sector (South Georgia), Indian Sector (Crozet and Kerguelen islands) of the Southern Ocean; • Define the habitat and trophic level of cephalopods in the Southern Ocean and adjacent waters, using stable isotope analyses; • Evaluate the implications of such findings on the conservation of wandering albatrosses.
20
2. MATERIAL AND METHODS
2.1 Study Area and sampling
The study area is focused on the Diomedea exulans’ breeding islands (Figure 1.1) off South Georgia (54ºS, 38ºW; South of the APF) and French archipelagos of Kerguelen (49ºS,69ºE; on the APF) (Moore et al., 1999; Koubbi et al . 1991) and Crozet (46ºS,51ºE; North of the APF) (Park et al., 1991; Belkin & Gordon, 1996; Park et al., 1997).
The cephalopod beaks were collected by two methods – boluses and induced regurgitations – both involving the sampling of stomach contents of albatrosses.
All samples were collected in the same year of 1998 (on the months of September, October and December).
The boluses were collected in South Georgia, where albatross chicks voluntarily regurgitate prior to the departure from the colony (fledgling) (Xavier et al., 2003a). Boluses comprise indigestible items, including beaks of cephalopods given by both parents to the chick, during the winter prior to its departure, from April/May until October/December (Prince & Morgan, 1987; Xavier et al., 2003b; Xavier & Croxall, 2007; Xavier et al., 2005).
The second sampling method – induced regurgitations (the animal is held upside down, and its chest is massaged until the stomach contents are vomited) – was used in the archipelagos of Crozet and Kerguelen. They were obtained immediately after the chicks being fed by one of its parents (Cherel & Weimerskirch, 1999; Weimerskirch et al., 2005).
2.2 Characterization of cephalopod component in the albatross’ diet
After sampling in 1998, samples were frozen at 20ºC, until laboratory treatment. Samples from Crozet and Kerguelen were analyzed in the Centre E´tudes Biologiques de Chizé in France, while the ones from South Georgia were analyzed at the British Antarctic Survey headquarters, Cambridge (UK).
The sample treatment was performed according to the procedures described in Table 2.1. The identification of lower beaks was done according to Xavier & Cherel (2009). Beak identification
21 was confirmed against the collections present in the British Antarctic Survey and in the Centre E´tudes Biologiques de Chizé.
Table 2.1 – Laboratory procedures adopted on the treatment of the different structures.
Structure Procedure Clean and separation in upper and lower beaks (Xavier et al . Beak 2003a). Upper beak Counted
Counted, measurement of lower rostral length (LRL) with callipers with a precision of a tenth of a millimeter and Lower beak identification to the species level when possible (Xavier et al., 2003a; Xavier & Cherel, 2009).
To characterize the cephalopod component in the wandering albatross diet, the following indices were determined for each island:
i. Weight index value (%W): indicates the percentage of weight that each prey species has in the diet. For that, it was used allometric equations that relate the wet mass (M, in grams) and Mantle Length (ML, in mm) with the Lower Rostral Length (LRL) of the squids, and the Lower Hood Length (LHL) in the octopuses (Xavier &Cherel, 2009). The total weight contribution of a certain species is then calculated by multiplying the mean weight of the individuals sampled and measured (LRL), with the total number of Lower beaks counted for that same species in the samples. Allometric equations from Xavier & Cherel 2009 were used (Table 7.1,in annex). No equation was available for the ML of Haliphron atlanticus ; ii. Numeric index value (%N): it is the number of prey of a certain species divided by the total number of prey in the samples. The number of prey was estimated by the number of lower beaks found on the samples; iii. Frequency index value (%F): percentage of samples with lower beaks of each prey.
Biological diversity of each sample was calculated using the Shannon Wienner index:
;
22
For comparison of diet diversity, there were plotted individual based rarefaction curves of each island and by confidence intervals, it was deliberated if the samples are equal or not. In this case, it was used a mathematically distinct but computationally much faster way, the “random placement” curve of Coleman (Coleman, 1981; Coleman et al., 1982), which has been shown to very closely approximate the hypergeometric rarefaction curve (Brewer & Williamson 1994; Colwell & Coddington 1994). Confidence Intervals of 95% were calculated by adding and subtracting to the curve the double of standard deviation registered in each point of the curve.
2.3 Stable isotopes analysis
After the characterization of the cephalopod component in the diet of wandering albatrosses off South Georgia, Crozet, and Kerguelen, only the cephalopod species that had at least 30 individuals present in one of the islands diets were used in the stable isotope study, ie., the species choice was done according to their importance by number and mass in the diets.
After that, 10 lower beaks for each species were randomly chosen following Cherel & Hobson (2005) procedure.
In IMAR CMA laboratory, the beaks were dried at 60ºC and grinded into a fine powder; 0.30 to 0.55 mg of each beak sample were placed in a tin capsule, and the stable isotope signatures were measured using a Flash EA 1112 Series elemental analyser coupled on line via Finningan conflo II interface to a Thermo delta V S mass spectrometer. Replicate measurements of internal laboratory standards (acetanilide) indicate measurement errors < 0.1 % both for Carbon and for Nitrogen.
The Carbon and Nitrogen isotope signatures are expressed in delta (δ) notation, defined as the parts per thousand (‰) deviation from a standard material (PDB limestone for δ 13C and atmospheric Nitrogen for δ 15N);
δ 13C or δ 15N , where R = 13C/12C or 15N/14N.
After this procedure, it was subtracted 0.75‰ and added 4.8‰ to the Carbon and Nitrogen signature, respectively, to obtain the mean soft tissues signature of the cephalopods (Cherel & Hobson, 2006).
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2.3.1 Isotope Modeling
Samples with δ 13C signatures above 19.5‰ and below 22.3‰ were considered of Subtropical and Antarctic origin respectively (Cherel & Hobson, 2007). Those that did not enter in these two groups, were Subantarctic.
Trophic levels (TL) of the samples were calculated according to Minagawa & Wada (1984) equation:
, using the δ 15N baseline as Salpa thompsoni with δ15N=3.0‰ (South Georgia average of Su7 and Su8 of (Stowasser et al., 2012)) and 3.4‰ (Crozet island and Kerguelen (Cherel et al, 2008)), both at TL=2 to compare later in this study with other top predators of the ocean. Subtropical species (with a δ 13C signatures above 19.5‰) were not included in this calculations, as they have a different d15N baseline of the other 2 oceanic areas (Subantarctic and Antarctic, I.e. below δ 13C= 19.5‰).
To estimate mean foraging latitude of D. exulans in each island, the means and standard deviation of the stable isotopes signatures of all cephalopod sampled were calculated. Afterwards, the Weighted mean Carbon and Nitrogen signature of the cephalopod component of the Wandering Albatross diet was calculated by weighting the mean signature of each species, with the number of individuals of each cephalopod found on the diet of D. exulans , for each island. Representation of the diet (total individuals of the sampled species for SI analysis on the diet/total individuals on the diet) is presented in %.
2.4 Statistical Analyses
In order to compare the three diet indexes, there were used chi squared tests. For that, individual categories were created for each common species to the three islands and all the others species that only occurred in one or two islands were merged in a category called “others”. This was due to the high sensibility of the chi squared test to null entries, skewing the test results to statistical significance.
24
For the frequency index analysis only the common species to the three islands categories were considered, because otherwise it would skew the final results.
Histioteuthis B is a group of species ( H. atlantica and H. eltaninae ) merged into this division, on the moment of identification and measurement of LRL by the British Antarctic Survey in 1998 (South Georgia sample). However, this 2 species were separated a posteriori , by determining H. eltaninae highest LRL value (4.2 mm inclusive), and higher values being of H. atlantica LRL, by the observation of LRL distribution of both these species in the other studied islands . This means, H. atlantica lower LRL values are included in the H. eltaninae sample.
The mean, standard deviation (presented in mean ± standard deviation) and range (minimum maximum) were calculated for LRL, stable isotopes signatures data and the mantle length and weight values of the species (note: the latter were calculated with LRL allometric equations). It was only used the LRL and Stable isotopes signatures to test for differences between cephalopods in different diets, due to the inherent error that the allometric equations used to calculate weight and length have.
Test for difference on previous parameters between two different islands was made by the use of T Test if assumptions are followed; If not, it was used the Mann Whitney test or Kruskall Wallis.
When comparing multiple islands (k>3) analysis was carried using an ANOVA (previously, normality and homogeneity of variances were verified) or Kruskall Wallis. If significant differences were demonstrated somewhere among the groups with the ANOVA or Kruskall Wallis tests, the Tukey or Dunn Tests were used, respectively, to find out where those differences were.
All statistical analyses were performed for a significance level of 0.05, using Statistica 10.0. EstimateS Win 8.20 software was used to calculate the values for the Coleman curves.
25
3. RESULTS
3.1 Overall
3.1.1 Diet
A total of 15,583 beaks were analyzed from the diet of 82 wandering albatrosses. Of those, 7677 were upper and 7906 were lower beaks, all comprising 53 different cephalopod species belonging to 22 families. The overall distribution of LRL of the beaks revealed three conspicuous peaks (2 to 3, 5 to 6 and 12 to 13 mm), and a forth minor one around 9 10 mm (Figure 3.1).
Figure 3.1 - Lower Rostral Length (LRL) distribution of the squids found on the diet of Wandering Albatross in South Georgia, Crozet and Kerguelen.
3.1.2 Stable isotopes
A total of 384 samples were collected from the 3 islands. The selected species for stable isotopes analysis (both Histioteuthis miranda and Teuthowenia pellucida were not included as they contributed poorly to the diets, whereas Haliphron atlanticus that had only 14 beaks entered the sampled species due to its cosmopolitan distribution, and interest for future studies) were responsible for a total of 94.1% of the beaks in Crozet (93.1% of the mass), 86.6% in Kerguelen
26
(71.9% in of the mass) and 94.9% in South Georgia (96.6% of the mass) (Table 3.10). The δN values varied between 7.21‰ ( Martialia hyadesi from Crozet) to 18.11‰ ( Gonatus antarcticus from South Georgia), and δ13C from 26.50‰ ( Kondakovia longimana of South Georgia) to 18.62‰ ( Histioteuthis atlantica from Kerguelen). Squid with less than 19.5‰ feed along a continuum of about 1 trophic level (4.77‰) from K. longimana (11.97±0.38‰ to 12.59±0.75‰) to T. sp. B (Voss) (15.75±0.80‰ to 16.74±0.64‰). This continuum was preceded by a drop of 2.71‰ (almost 1 trophic level) to M. hyadesi (8.4±0.84‰ and 9.26±0.45‰). All this are followed by a second feed continuum consisting of subtropical species that span less than 1 trophic level (1.93‰), beginning at H. atlantica small (15.07±0.97‰), and ending at C. akimushkini (17±0.52‰).
3.2 South Georgia
3.2.1 Diet
A total of 1421 upper and 1329 lower beaks were found in the samples (n= 19) from South Georgia. The distribution of LRL of the beaks is shown in Figure 3.2 and Table 3.1. Four peaks were observed, namely:
i. 3 to 4 mm, due to the great amount of Histioteuthis eltaninae beaks; ii. 5 to 6 mm, the largest peak, which was composed by Alluroteuthis antarcticus , G. antarticus and H. atlantica ; iii. 9 to 10 mm, due to the presence of Taonius sp. B (Voss); iv. 14 to 15 mm, due to the presence of K. longimana .
A total of 28 cephalopod species were identified, of which 3 were only found in this island. The Shannon Wienner value was H= 0.998. The most numerous preys found were (by number) K. longimana (24.2%), T. sp . B (Voss) (23.7%), H.eltaninae (10.6%), A. antarcticus (7.9%), G. antarcticus (6.8%) and H.atlantica (5.7%) (Table 3.2). In terms of mass, K. longimana (75.5%) and T. sp . B (Voss) (7.9%) were the most important (Table 3.2). The distribution of the mantle length and weigth of each species is shown in Table 3.1 & Table 7.2 , in annex. Mantle length ranged from 47.2 mm (in Histioteuthis macrohista ) up to 706.8 mm (in Taningia danae ), while the weight values showed that the lightest prey came from from Brachioteuthis ?picta and Batoteuthis skolops (7.8 g ) and the heaviest was again, T. danae (6471.2 g ).
27
Figure 3.2 – Lower Rostral Length (LRL) distribution of the squids found on the diet of Wandering Albatross in South Georgia.
28
Table 3.1 - Lower Rostral Length (LRL), Mantle Length (ML) and Weight (W) of the main species found on the diet of Wandering Albatrosses of South Georgia, Crozet islands and Kerguelen. (Continued next page)
South Georgia
LRL (mm) ML (mm) W (g)
mean ± sd mean ± sd mean ± sd
(Range) (Range) (Range)
Haliphron 12.51 ± 2.92 - 482.63 ± 165.14 Alloposidae atlanticus 7.90 - 18.60 - 243.95 - 844.36
Architeuthis - - - Architeuthidae dux
Batoteuthis 4.17 ± 0.71 113.37 ± 17.36 39.59 ± 20.77 Batoteuthidae skolops 3.00 - 6.30 84.78 - 165.50 15.26 - 113.12
Galiteuthis 5.30 ± 0.48 450.60 ± 40.48 102.98 ± 20.45
glacialis 4.00 - 6.40 341.82 - 542.90 54.89 - 154.38
Taonius - - - Cranchidae sp.(Clarke)
Taonius sp.B 9.24 ± 1.08 555.30 ± 66.31 290.90 ± 69.66
(Voss) 5.40 - 11.30 319.42 - 681.86 88.17 - 444.22
Cycloteuthis - - - Cycloteuthidae akimushkini
Gonatus 6.05 ± 0.96 215.94 ± 41.25 228.12 ± 112.49 Gonatidae antarcticus 3.40 - 8.20 102.36 - 308.13 30.57 - 573.51
Histioteuthis 5.51 ± 0.55 130.95 ± 14.07 295.28 ± 70.41
atlantica 4.30 - 6.70 99.92 - 161.50 158.16 - 468.79
Histioteuthis 3.46 ± 0.29 81.01 ± 7.06 67.44 ± 17.25 Histioteuthidae eltaninae 2.30 - 4.20 52.65 - 99.17 18.55 - 120.68
Histioteuthis 5.63 ± 0.63 134.13 ± 16.09 468.77 ± 157.70
miranda 4.70 - 6.50 110.18 - 156.37 261.02 - 699.44
Mastigoteuthis 6.93 ± 0.82 181.02 ± 20.16 151.27 ± 49.49 Mastigoteuthidae sp.A (Clarke) 5.00 - 9.60 133.70 - 246.22 60.61 - 352.75
Alluroteuthis 5.16 ± 0.48 176.10 ± 16.88 437.86 ± 120.04 Neoteuthidae antarcticus 3.40 - 6.70 114.67 - 230.13 125.44 - 924.09
Martialia 4.40 ± 0.46 231.67 ± 13.50 219.93 ± 46.52 Ommastrephidae hyadesi 4.00 - 4.90 219.88 - 246.40 180.23 - 271.11
29
Kondakovia 13.45 ± 1.72 479.46 ± 64.04 2709.54 ± 978.52
longimana 5.30 - 17.50 175.44 - 630.72 136.78 - 5903.99
Moroteuthis 9.90 377.07 1729.76 ingens Onychoteuthidae Moroteuthis 6.87 ± 0.96 322.81 ± 60.09 695.41 ± 424.50
knipovitchi 5.40 - 9.40 231.09 - 480.56 250.62 - 2057.44
Moroteuthis 7.87 ± 0.31 535.19 ± 46.14 1852.95 ± 595.67
robsoni 7.60 - 8.20 494.92 - 585.54 1362.61 - 2515.84
Taningia 14.70 ± 3.21 548.83 ± 241.76 4609.20 ± 2693.68 Octopoteuthidae danae 11.00 - 16.80 270.52 - 706.80 1520.51 - 6471.19
Crozet
LRL (mm) ML (mm) W (g)
mean ± sd mean ± sd mean ± sd
(Range) (Range) (Range)
Haliphron Alloposidae - - - atlanticus Architeuthis Architeuthidae 8.53 450.31 3050.94 dux
Batoteuthis 4.02 ± 0.45 109.82 ± 11.02 34.66 ± 10.12 Batoteuthidae skolops 3.01 - 4.96 85.02 - 132.72 15.40 - 59.31
Galiteuthis 5.38 ± 0.35 457.83 ± 29.49 106.17 ± 14.93
glacialis 4.01 - 6.26 342.65 - 531.17 55.20 - 147.05
Taonius 5.12 ± 0.29 302.21 ± 17.55 78.76 ± 9.56 Cranchidae sp.(Clarke) 4.52 - 5.69 265.36 - 337.24 59.72 - 98.87
Taonius sp.B 8.65 ± 1.20 518.86 ± 73.76 253.30 ± 77.59
(Voss) 5.74 - 11.60 340.31 - 700.29 100.78 - 470.46
Cycloteuthis 12.76 ± 2.55 395.42 ± 78.90 982.31 ± 350.48 Cycloteuthidae akimushkini 6.39 - 17.56 198.09 - 544.36 246.34 - 1768.64
Gonatus 6.05 ± 0.64 215.75 ± 27.40 217.17 ± 87.61 Gonatidae antarcticus 5.05 - 7.89 173.09 - 294.84 114.16 - 504.43
Histioteuthis 5.64 ± 0.84 134.36 ± 21.44 319.44 ± 107.39
atlantica 3.20 - 7.20 71.69 - 174.33 76.69 - 559.20
Histioteuthis 3.46 ± 0.32 80.98 ± 7.90 67.73 ± 19.15 Histioteuthidae eltaninae 2.30 - 5.03 52.65 - 119.48 18.55 - 211.44
Histioteuthis 6.84 ± 0.40 207.56 ± 13.77 825.91 ± 146.34
miranda 5.91 - 7.71 175.67 - 237.25 523.74 - 1175.27
Mastigoteuthidae Mastigoteuthis 6.62 ± 0.62 194.26 ± 18.06 284.07 ± 72.31
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sp.A (Clarke) 5.26 - 7.79 154.76 - 228.33 143.33 - 444.16
Alluroteuthis 5.46 ± 0.38 186.70 ± 13.23 512.31 ± 100.55 Neoteuthidae antarcticus 4.22 - 6.23 143.36 - 213.69 236.96 - 745.97
Martialia 6.81 ± 0.83 302.57 ± 23.31 532.83 ± 128.64 Ommastrephidae hyadesi 5.17 - 9.00 254.36 - 367.23 302.01 - 921.33
Kondakovia 12.58 ± 1.37 447.30 ± 51.13 2174.27 ± 796.43
longimana 6.20 - 18.66 209.02 - 674.01 224.24 - 7227.75
Moroteuthis 8.70 ± 1.04 343.04 ± 47.65 1397.23 ± 683.18
ingens 5.82 - 11.67 236.25 - 492.99 413.88 - 4149.35 Onychoteuthidae Moroteuthis 7.30 ± 0.84 349.35 ± 52.26 840.84 ± 354.75
knipovitchi 5.75 - 9.07 252.91 - 459.98 318.13 - 1796.30
Moroteuthis 8.86 ± 0.39 685.22 ± 59.50 4883.08 ± 1823.92
robsoni 8.54 - 9.30 636.89 - 751.67 3491.97 - 6948.05
Taningia 15.07 ± 1.72 576.67 ± 129.49 4659.38 ± 1699.85 Octopoteuthidae danae 12.21 - 17.41 361.54 - 752.68 2172.67 - 7310.69
Kerguelen
LRL (mm) ML (mm) W (g)
mean ± sd mean ± sd mean ± sd
(Range) (Range) (Range)
Haliphron - - - Alloposidae atlanticus
Architeuthis 11.16 ± 2.85 606.10 ± 168.75 15815.86 ± 16350.63 Architeuthidae dux 7.67 - 15.41 399.31 - 858.37 1877.20 - 45525.42
Batoteuthis 4.71 ± 0.57 126.62 ± 13.82 53.24 ± 16.51 Batoteuthidae skolops 3.67 - 5.57 101.17 - 147.64 26.30 - 81.12
Galiteuthis 5.45 ± 0.33 463.27 ± 27.39 108.90 ± 13.91
glacialis 3.84 - 6.29 328.41 - 533.68 50.18 - 148.60
Taonius 4.98 ± 0.22 293.70 ± 13.59 74.07 ± 7.17 Cranchidae sp.(Clarke) 4.56 - 5.40 267.82 - 319.42 60.88 - 88.17
Taonius sp.B 9.62 ± 1.09 578.55 ± 66.83 317.28 ± 74.70
(Voss) 6.64 - 11.73 395.60 - 708.27 138.64 - 482.08
Cycloteuthis 12.78 ± 2.31 396.29 ± 71.57 980.75 ± 322.37 Cycloteuthidae akimushkini 6.90 - 17.98 213.90 - 557.38 286.14 - 1852.07
Gonatus 6.37 ± 0.73 229.64 ± 31.28 259.97 ± 105.19 Gonatidae antarcticus 5.37 - 7.98 186.81 - 298.70 140.07 - 523.85
Histioteuthis 6.05 ± 0.75 144.71 ± 19.10 374.03 ± 101.80 Histioteuthidae atlantica 2.54 - 7.79 54.76 - 189.47 43.55 - 678.21
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Histioteuthis 3.22 ± 0.29 75.23 ± 7.07 54.33 ± 15.60
eltaninae 2.51 - 4.05 57.79 - 95.49 24.34 - 107.77
Histioteuthis 6.41 ± 1.03 192.63 ± 35.11 715.27 ± 252.18
miranda 2.85 - 7.80 70.99 - 240.33 57.05 - 1217.48
Mastigoteuthis 6.84 ± 0.95 200.60 ± 27.66 319.01 ± 113.27 Mastigoteuthidae sp.A (Clarke) 4.76 - 8.08 140.22 - 236.77 107.50 - 493.46
Alluroteuthis 5.41 ± 0.40 184.93 ± 14.05 499.36 ± 102.55 Neoteuthidae antarcticus 4.17 - 6.10 141.61 - 209.14 228.79 - 701.07
Martialia 5.97 ± 0.81 278.05 ± 23.77 411.22 ± 111.97 Ommastrephidae hyadesi 4.36 - 7.68 230.49 - 328.33 214.35 - 669.61
Kondakovia 13.44 ± 1.52 479.37 ± 56.57 2685.82 ± 1034.12
longimana 10.26 - 19.04 360.53 - 688.19 1097.05 - 7701.93
Moroteuthis 10.49 ± 0.85 440.15 ± 38.11 2986.58 ± 741.94
ingens 9.21 - 11.33 383.20 - 477.82 1922.40 - 3769.18 Onychoteuthidae Moroteuthis 6.94 ± 0.75 327.06 ± 46.80 691.11 ± 303.82
knipovitchi 5.80 - 8.79 256.03 - 442.52 328.77 - 1594.62
Moroteuthis 9.17 ± 0.58 731.55 ± 88.04 6883.91 ± 3446.28
robsoni 8.32 - 10.12 603.66 - 875.51 2828.79 - 13740.81
Taningia 17.36 ± 2.17 748.56 ± 163.14 7656.06 ± 2669.42 Octopoteuthidae danae 11.62 - 20.62 317.16 - 994.14 1834.14 - 13040.49
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Table 3.2 - Frequency of occurrence (F%), number of beaks (N%) and estimated mass(W%) of the main species contributing to the diet of Wandering Albatross in South Georgia, Crozet and Kerguelen. All species in Table 7.3 in annex.
South Georgia Crozet Kerguelen
Family Species F% N% W% F% N% W% F% N% W%
Alloposidae Haliphron atlanticus 52.6 1.1 0.6 ------
Architeuthidae Architeuthis dux - - - 12.1 0.1 0.3 63.3 0.8 15.0
Batoteuthidae Batoteuthis skolops 57.9 2.2 0.1 84.8 2.8 0.1 66.7 1.3 0.1
Galiteuthis glacialis 84.2 4.5 0.5 97.0 8.8 1.0 96.7 12.2 1.5
Cranchidae Taonius sp.(Clarke) - - - 48.5 1.0 0.1 60 2.1 0.2
Taonius sp. B (Voss) 100.0 23.7 7.9 57.6 1.6 0.4 53.3 6.8 2.5
Cycloteuthidae Cycloteuthis akimushkini - - - 57.6 1.0 1.0 86.7 3.2 3.6
Gonatidae Gonatus antarcticus 89.5 6.8 1.8 60.6 1.5 0.3 73.3 1.7 0.5
Histioteuthis atlantica 89.5 5.8 2.0 84.8 3.3 1.1 96.7 29.9 12.9
Histioteuthidae Histioteuthis eltaninae 100.0 10.6 0.8 100.0 25.3 1.8 86.7 7.9 0.5
Histioteuthis miranda 42.1 0.9 0.5 54.5 0.9 0.7 60.0 1.4 1.2
Mastigoteuthidae Mastigoteuthis sp.A (Clarke) 78.9 3.9 0.7 54.5 0.8 0.2 23.3 0.4 0.2
Neoteuthidae Alluroteuthis antarcticus 94.7 8.0 4.0 87.9 2.5 1.3 90.0 3.2 1.9
Ommastrephidae Martialia hyadesi 10.5 0.2 0.1 84.8 4.3 2.4 86.7 3.7 1.8
Kondakovia longimana 94.7 24.2 75.5 100.0 33.7 76.0 86.7 10.0 31.0
Moroteuthis ingens 5.3 0.1 0.1 93.9 4.1 5.9 20.0 0.3 0.9 Onychoteuthidae Moroteuthis knipovitchi 68.4 3.2 2.6 93.9 3.4 3.0 83.3 2.5 2.0
Moroteuthis robsoni 10.5 0.2 0.5 9.1 0.1 0.4 46.7 0.9 6.8
Octopoteuthidae Taningia danae 10.5 0.2 1.2 18.2 0.2 0.7 46.7 1.5 13.2
3.2.2 Stable isotopes 119 beaks from South Georgia were used for stable isotopes analysis. The δN values ranged from 11.25‰ ( K. longimana ) to 18.11‰ ( G. antarcticus ), and δ13C from 26.50‰ ( K. longimana ) to 19.20‰ ( H. atlantica small) The distribution of the δ15N and δ13C signatures by species is showed in the Table 3.3 and Figure 3.3. There were three δ15N signatures groups: i) K. longimana was the squid with by far the lowest signature (11.97±0.38‰) followed by ii) the second group, consisting of a continuum of squids beginning at G. glacialis (13.39±1.10‰) and finishing at B. skolops (14.45±0.28‰), iii) and finally, a second continuum of squids, starting with H. atlantica small (15.89±0.58‰), and ending at H. atlantica large(16.75±0.72‰). The highest standard deviations were found in G. glacialis (1.10‰) and A. antarcticus (0.98‰).
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Subtropical signatures (mean δ13C higher than 19.5‰) were not found, but H. atlantica showed the closest values as it had the highest values for δ13C ( 19.9±0.48‰ and 20.39±0.61‰ for small and large specimens respectively).Antarctic signatures (below 22.3‰) were found in H. eltaninae ( 22.66±1.20‰), G. antarcticus ( 23.28±2.33‰), M. knipovitchi ( 23.85±1.00‰), K. longimana ( 24.37±1.59‰) and B. skolops ( 25.14±0.54‰). The species showing high standard deviations in their δ13C signatures were G. antarcticus (2.33‰), A. antarcticus (1.46‰), K. longimana (1.59‰), H. eltaninae (1.20‰) and M. knipovitchi (1‰).
Table 3.3 - Lower Rostral Length (LRL), Nitrogen and Carbon stable isotopes signatures of the main species found on the diet of Wandering Albatrosses of South Georgia.
South Georgia LRL(mm) Nitrogen (‰) Carbon (‰) Family Species mean ± sd mean ± sd mean ± sd
Alloposidae Haliphron atlanticus 12.51 ± 2.92 13.80 ± 0.41 -20.91 ± 0.30
Batoteuthidae Batoteuthis skolops 4.17 ± 0.71 14.45 ± 0.28 -25.14 ± 0.54
Galiteuthis glacialis 5.30 ± 0.48 13.39 ± 1.10 -22.27 ± 0.82
Cranchidae Taonius sp. (Clarke) ------
Taonius sp. B (Voss) 9.24 ± 1.08 16.74 ± 0.64 -21.94 ± 0.82
Cycloteuthidae Cycloteuthis akimushkini ------
Gonatidae Gonatus antarcticus 6.05 ± 0.96 16.46 ± 0.73 -23.28 ± 2.33
Histioteuthis atlantica 5.51 ± 0.55 16.34 ± 0.78 -20.17 ± 0.59
Histioteuthis atlantica - - 15.89 ± 0.58 -19.92 ± 0.48 small Histioteuthidae Histioteuthis atlantica - - 16.75 ± 0.72 -20.39 ± 0.61 Large Histioteuthis eltaninae 3.46 ± 0.29 14.28 ± 0.76 -22.66 ± 1.20
Histioteuthis miranda ------
Mastigoteuthis sp. A Mastigoteuthidae 6.93 ± 0.82 15.95 ± 0.46 -21.26 ± 0.75 (Clarke) Neoteuthidae Alluroteuthis antarcticus 5.16 ± 0.48 13.52 ± 0.98 -21.67 ± 1.46
Ommastrephidae Martialia hyadesi ------
Kondakovia longimana 13.45 ± 1.72 11.97 ± 0.38 -24.37 ± 1.59
Onychoteuthidae Moroteuthis ingens ------
Moroteuthis knipovitchi 6.87 ± 0.96 13.88 ± 0.63 -23.85 ± 1.00
Octopoteuthidae Taningia danae ------
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