Literature DB >> 26696769

Southern Ocean Asteroidea: a proposed update for the Register of Antarctic Marine Species.

Camille Ve Moreau1, Antonio Aguera1, Quentin Jossart1, Bruno Danis1.   

Abstract

BACKGROUND: The Register of Antarctic Marine Species (RAMS, De Broyer et al. 2015) is the regional component of the World Register of Marine Species (WoRMS Editorial Board 2015) in the Southern Ocean. It has been operating for the last ten years, with a special effort devoted towards its completion after the International Polar Year (IPY) in 2007-2008, in the framework of the Census of Antarctic Marine Life (CAML, 2005 - 2010). Its objective is to offer free and open access to a complete register of all known species living in the Southern Ocean, building a workbench of the present taxonomic knowledge for that region. The Antarctic zone defined by this dynamic and community-based tool has been investigated with a particular interest. The Sub-Antarctic zone was a secondary objective during the establishment of the RAMS and is still lacking the impulse of the scientific community for some taxa. NEW INFORMATION: In the present study, more than 13,000 occurrences records of Asteroidea (Echinodermata) have been compiled within the RAMS area of interest and checked against the RAMS species list of sea stars, using WoRMS Taxon Match tool. Few mismatches (basionym mistakes : i.e. original name misspelled or incorrect) were found within the existing list and 97 unregistered species are actually occurring within the RAMS boundaries. After this update, the number of Asteroidea species was increased by around 50%, now reaching 295 accepted species.

Entities:  

Keywords:  Asteroidea; Biodiversity; RAMS; Sea stars; WoRMS;  Checklist;  Register of Antarctic Marine Species;  Southern Ocean

Year:  2015        PMID: 26696769      PMCID: PMC4678801          DOI: 10.3897/BDJ.3.e7062

Source DB:  PubMed          Journal:  Biodivers Data J        ISSN: 1314-2828


Introduction

The Register of Antarctic Marine Species, RAMS

RAMS is a collaborative and dynamic information system managing Southern Ocean marine taxon names and related information (De Broyer et al. 2015). The main objective of RAMS is to establish a benchmark of the present taxonomic knowledge of the Southern Ocean biodiversity (De Broyer et al. 2011). In a recent appraisal of RAMS, Jossart et al. (2015)​ underscored the number of 10,294 described species of which 8,297 are accepted marine species (viz. checked by taxonomic experts). Among these species, 537 (~6.5%) were reported as accepted species names for echinoderms and 198 (~2.4%) as accepted names for sea star species. After 10 years of service, RAMS still displays several spatial gaps, especially with regards to species occurring in the sub-Antarctic zone, described as the area below the sub-Tropical front (Deacon 1984, Rintoul 2007) and North of the Polar Front. In order to complete the taxonomic information for the class , we propose in this work an updated version of the checklist of Southern Ocean sea stars species occurring within the RAMS area of interest.

Materials and methods

Area of interest

As described in De Broyer and Danis (2011) the RAMS area of interest is extending from the coast of the Antarctic continent to the sub-Tropical front. Convenient operational limits have been defined (Table 1; Fig. 1), splitting the Southern Ocean into two zones: the Antarctic zone and the sub-Antarctic zone.
Table 1.

RAMS area of interest. Operational northern limits in the different sector of the Southern Ocean for both the Antarctic zone and the sub-Antarctic zone.

Sector Longitude range Northern limit
Antarctic zone
South Atlantic Sector60°W-50°W57°S
50°W-30°E50°S
Indian Sector30°E-80°E50°S
80°E-150°E55°S
South Pacific Sector150°E-60°W60°S
Sub-Antarctic zone
Atlantic & Indian Sectors60°W-140°E43°S
South Pacific Sector140°E-176°W48°S
176°W-80°W45°S
80°W-72°W41°S
Figure 1.

Occurrences of RAMS (light grey dots) and Proposed-RAMS (orange dots) sea star species. The Antarctic zone is located below the green line and the Sub-Antarctic zone between the green and dark red lines. The Polar Front (black line) and the Sub-Tropical Front (dashed black line) are also shown.

Data collection

More than 13,000 occurrences records were agregated from different sources including global information systems such as the Ocean Biogeographic Information System (OBIS), the Global Biodiversity Information Facility (GBIF), initiatives such as the Biogeographic Atlas of the Southern Ocean (De Broyer et al. 2014), historic records mined from the literature pertaining to the early exploration of the Southern Ocean (e.g. Sladen 1889), recently published checklists (e.g. Gutt et al. 2014) or unpublished cruise records. Only the specimens identified at a species level, regardless of their depth (shelf, slope, deep-sea)  were kept for the preparation of this checklist. The validity of each species name was controlled using the Taxa Match Tool available in RAMS (http://www.marinespecies.org/rams/aphia.php?p=match) and WoRMS (http://www.marinespecies.org/aphia.php?p=match) to ensure its validity and presence in the RAMS checklist.

Data resources

Complete checklist of Southern Ocean Asteroidea

The data underpinning the analyses reported in this paper are deposited at GBIF, the Global Biodiversity Information Facility, http://ipt.pensoft.net/resource?r=southern_ocean_asteroidea&v=1.1

Checklists

Checklist of RAMS species

(Sladen, 1883) (Sladen, 1883) (Koehler, 1912) (Koehler, 1920) (Sladen, 1889) (Bell, 1908) (Koehler, 1912) (Koehler, 1906) (Perrier, 1875) (Lütken, 1857) Perrier, 1875 (Koehler, 1920) (Koehler, 1920) Koehler, 1923 (E. A. Smith, 1876) (Verrill, 1876) (Koehler, 1920) (Bell, 1881) Perrier, 1891 (deLoriol, 1894) Fisher, 1940 Fisher, 1940 (E. A. Smith, 1876) Perrier, 1875 Müller & Troschel, 1842 Sladen, 1889 Ludwig, 1903 (Sladen, 1885) Clark, 1962 Bernasconi, 1966 Bernasconi, 1972 (Perrier, 1881) (Sladen, 1889) (Koehler, 1907) Ludwig, 1903 (Studer, 1884) (Sladen, 1889) Sladen, 1889 (H.E.S. Clark, 1971) Koehler, 1908 H.L. Clark, 1923 Fisher, 1940 (Philippi, 1858) Sladen, 1889 Koehler, 1923 (Koehler, 1906) Lütken, 1871 Sladen, 1889 (Koehler, 1912) (Koehler, 1917) Koehler, 1920 (Philippi, 1857) (Bell, 1881) (Koehler, 1908) (Koehler, 1917) (Perrier, 1875) (Studer, 1885) (Koehler, 1923) (Müller & Troschel, 1843) Bernasconi, 1937 (Sladen, 1882) (Sladen, 1882) (Sladen, 1882) Koehler, 1907 Ludwig, 1903 (Sladen, 1883) (Ludwig, 1905) Ludwig, 1907 (Sladen, 1889) Sladen, 1889 Döderlein, 1927 Korovchinsky, 1976 Sladen, 1889 Koehler, 1908 Sladen, 1889 Korovchinsky, 1976 Koehler, 1907 Gray, 1847 Perrier, 1891 (Sladen, 1889) (E. A. Smith, 1876) (Studer, 1885) (Koehler, 1923) A.M. Clark, 1962 (Sladen, 1889) (Studer, 1885) Koehler, 1912 (Sladen, 1889) (Koehler, 1920) Perrier, 1891 Fisher, 1940 (Parelius, 1768) Sladen, 1882 Koehler, 1908 Sladen, 1882 Sladen, 1882 Koehler, 1908 Koehler, 1908 Sladen, 1882 Koehler, 1908 Sladen, 1882 Sladen, 1882 Thomson, 1873 Ludwig, 1903 Sladen, 1882 Sladen, 1882 (Sladen, 1889) Sladen, 1883 Koehler, 1907 Koehler, 1920 A.M. Clark, 1962 Sladen, 1889 Lütken, 1872 (Koehler, 1920) E. A. Smith, 1876 (Koehler, 1912) (Bernasconi, 1969) Fisher, 1923 Sladen, 1889 Fisher, 1940 Koehler, 1912 Sladen, 1889 Koehler, 1920 (Say, 1825) (Koehler, 1920) (Ludwig, 1903) (Ludwig, 1903) A.M. Clark, 1962 Fisher, 1940 Fisher, 1940 (Koehler, 1920) (Ludwig, 1903) (Studer, 1885) (Koehler, 1920) (Perrier, 1881) Fisher, 1940 (Studer, 1885) (Studer, 1885) (Koehler, 1911) (Koehler, 1912) (Ludwig, 1903) Koehler, 1920 (Koehler, 1907) Fisher, 1940 Fisher, 1940 (H.E.S. Clark, 1962) Fisher, 1940 (E. A. Smith, 1876) (Philippi, 1870) Koehler, 1907 Koehler, 1906 (Koehler, 1912) (Koehler, 1912) (Koehler, 1907) Perrier, 1885 Sladen, 1889 (Bell, 1908) H.E.S. Clark, 1963 Sladen, 1889 Koehler, 1920 (Koehler, 1906) Koehler, 1912 (Koehler, 1920) (Koehler, 1912) Sladen, 1889 Sladen, 1889 (Perrier, 1891) (Koehler, 1907) Perrier, 1891 Wyville Thomson, 1877 Fisher, 1940 Sladen, 1889 (Koehler, 1906) Smith, 1876 Koehler, 1920 (Sladen, 1882) (Sladen, 1882) A.M. Clark, 1962 Sladen, 1882 (Sladen, 1882) Sladen, 1882 (H.L. Clark, 1916) Koehler, 1912 (Koehler, 1920) Koehler, 1920 Koehler, 1907 O'Loughlin & O'Hara, 1990 (Sladen, 1889) (Sladen, 1889) Downey, 1971 Sladen, 1889 Sladen, 1883 Ludwig, 1907 Sladen, 1883 Koehler, 1908 Verrill, 1880 Bernasconi, 1965 Sladen, 1889

Checklist of Proposed-RAMS species

McKnight, 2006 (Farquhar, 1895) (Muller & Troschel, 1844) (Hutton, 1879) (Sladen, 1889) (Mortensen, 1925) Müller & Troschel, 1842 (Hutton, 1872) H.E.S. Clark, 1969 H.E.S. Clark, 1969 McKnight, 1973 (Verrill, 1894) H.E.S. Clark, 2001 Studer, 1883 Mah, 2011 Mah & Foltz, 2014 (Gray, 1840) Verrill, 1870 H.L. Clark, 1916 McKnight, 1973 H.L. Clark, 1916 (Perrier, 1875) (Fell, 1953) McKnight, 1973 (H.L. Clark, 1916) Benham, 1909 Mah, 2011 (Sladen, 1889) Sladen, 1889 (Sladen, 1889) (Perrier, 1869) Fisher, 1906 Mortensen, 1925 (Sladen, 1889) (Farquhar, 1898) (Perrier, 1869) Fell, 1958 (Sladen, 1889) (E. A. Smith, 1876) McKnight, 1973 Wyville Thomson, 1876 (McKnight, 1973) (Döderlein, 1927) Macan, 1938 McKnight, 1973 A.H. Clark, 1917 (Sladen, 1889) McKnight, 1973 Benham, 1909 (O'Loughlin, Waters & Roy, 2003) (O'Loughlin, Waters & Roy, 2003) (Sladen, 1889) (Moyana & Larrain Prat, 1976) McKnight, 1973 (Mortensen, 1925) Janosik & Halanych, 2010 Janosik & Halanych, 2010 O'Hara, 1998 Rowe & Albertson, 1988 H.L. Clark, 1916 H.E.S. Clark, 1970 (Koehler, 1920) (Verrill, 1867) Mah et al. 2015 (Sladen, 1889) Gray, 1840 Fell, 1958 McKnight, 1973 (McKnight, 1973) McKnight, 2006 H.E.S Clark & D.G. McKnight, 2000 H.E.S. Clark, 1970 H.E.S Clark & D.G. McKnight, 2000 H.E.S Clark & D.G. McKnight, 2000 Fell, 1958 A.H. Clark, 1917 (Mortensen, 1925) McKnight, 2006 Fell, 1958 H.E.S. Clark, 1962 Sladen, 1889 Fell, 1958 McKnight, 1973 (Sladen, 1889) (Hutton, 1872) H.L. Clark, 1928 Stampanato & Jangoux, 1993 Sladen, 1889 A.M. Clark, 1976 (Verrill, 1871) McKnight, 1973 Sladen, 1889 Fisher, 1919 McKnight, 2006 Thomson, 1873 H.L. Clark, 1916 Fisher, 1906

Analysis

More than 13,000 occurrences records from 295 accepted species have been compiled within the extent of the RAMS area of interest. 198 of these species (67%) were already in the RAMS database and 97 (33%) were new to the system. After this update, the number of species in RAMS will be increased by around 50%. The seven Orders of the Class are represented in the Southern Ocean. The  are the most speciose with 8 families, 41 genus and 87 species followed by (6 families, 30 genus, 78 species), (6 families, 22 genus, 43 species), (2 families, 6 genus, 37 species), (1 family, 4 genus, 20 species), (2 families; 9 genus; 19 species) and  (1 family, 4 genus, 2 subgenus, 11 species). After a careful verification of the RAMS species list for we propose to address the following points. These issues have been taken into account in this paper: and  are only described from Central America and should be removed from the RAMS list is only described from Amsterdam and Saint-Paul Islands which are not part of the RAMS area of interest , , , , and do not seem to be distributed in the RAMS area of interest is only described from South America and should be removed of the RAMS list​ was originally described as  by Korovchinsky (1976) and are source of a problem. Both genus do exist but and are the only described species. The genus name being nearly identical, it has lead to a mistake.  is an invalid name and should be deleted from RAMS and WoRMS systems Moreover, we recommend the addition of species from our "Proposed-RAMS" checklist (i.e. species not registered in the RAMS list but present in the RAMS area of interest) to RAMS. None of these species are new to science but their austral distribution range was not properly documented (e.g. species from the Campbell Plateau are reported as New-Zealand species but are also present in the Southern Ocean, species from the French sub-Antarctic Islands, etc...). Interestingly, 22 of the 97 "non-RAMS" species are present in the Antarctic zone. Some have been described recently (e.g. and  described by Janosik and Halanych (2010);  described by Mah (2011) or  described by Mah et al. 2015) but have not been added to the RAMS. A final comment pertains to , occurring in the RAMS Sub-Antarctic region in a location that is not actually South from the Sub-Tropical Front. This final observation shows that convenient boundaries should be used with care. However, only one species was concerned for a very wide area of interest.  presence in the RAMS checklist should be discussed by the editors from RAMS and WoRMS.

Discussion

This study highlights the fact that after ten years of effort, the work is still in progress for RAMS. The main objective of covering the Antarctic zone has generally been reached for the class but needs at this point to go through a major update by the editors. Regarding the asteroids, the secondary objective of covering the Sub-Antarctic zone lacked the impulse of the scientific community and we hope that the work presented here will fill the gaps as accurately as possible. This approach may not bring the same results for all the taxa in the Southern Ocean. Indeed some charismatic fauna are very well known in the RAMS area of interest (e.g. marine mammals), however, we believe that the knowledge concerning the number of species present in the Southern Ocean waters might be significantly increased. Only few mistakes were found in the existing RAMS list of and should be fixed soon after getting in contact with the editors. The new updated checklist of species will be available through the RAMS website (http://www.marinespecies.org/rams) in early 2016. A way to improve the general system, with the sea stars for model is also in development. Recent work using genetics on  species (Janosik and Halanych 2010) highlights the fact that diversity might be higher than expected even in well-studied areas. There is also a lack of ressources for identification and taxonomic work leading to redundant mistakes. In this context, the creation of a digital library, hotlinked with the RAMS and compiling original descriptions, literature materials and DNA barcoding informations for each species will bring the RAMS a step ahead and provide a vital tool for future taxonomic and biogeographic work. Perspectives also include an illustrative determination key using a polytomic approach and the creation of interactive Antarctic Field Guides (http://afg.biodiversity.aq) on the http://www.biodiversity.aq platform (Van de Putte et al. 2015) in order to help the scientific community with the identification process and to enhance data availability. We believe that the homogenization of available data for all taxa will result in a better understanding of the Southern Ocean and its biogeography, especially in the Sub-Antarctic zone.
  3 in total

1.  Unrecognized Antarctic biodiversity: a case study of the genus Odontaster (Odontasteridae; Asteroidea).

Authors:  Alexis M Janosik; Kenneth M Halanych
Journal:  Integr Comp Biol       Date:  2010-09-03       Impact factor: 3.326

2.  The Register of Antarctic Marine Species (RAMS): a ten-year appraisal.

Authors:  Quentin Jossart; Camille Moreau; Antonio Agüera; Claude De Broyer; Bruno Danis
Journal:  Zookeys       Date:  2015-09-30       Impact factor: 1.546

3.  Asteroids, ophiuroids and holothurians from the southeastern Weddell Sea (Southern Ocean).

Authors:  Julian Gutt; Dieter Piepenburg; Joachim Voß
Journal:  Zookeys       Date:  2014-08-14       Impact factor: 1.546

  3 in total
  2 in total

1.  Antarctic and Sub-Antarctic Asteroidea database.

Authors:  Camille Moreau; Christopher Mah; Antonio Agüera; Nadia Améziane; Guillaume Crokaert; Marc Eléaume; Huw Griffiths; Lenaïg G Hemery; Anna Jażdżewska; Katrin Linse; Kate Neill; Chester Sands; Stefano Schiaparelli; Jacek Siciński; Noémie Vasset
Journal:  Zookeys       Date:  2018-04-02       Impact factor: 1.546

2.  Is reproductive strategy a key factor in understanding the evolutionary history of Southern Ocean Asteroidea (Echinodermata)?

Authors:  Camille Moreau; Bruno Danis; Quentin Jossart; Marc Eléaume; Chester Sands; Guillaume Achaz; Antonio Agüera; Thomas Saucède
Journal:  Ecol Evol       Date:  2019-07-16       Impact factor: 2.912

  2 in total

北京卡尤迪生物科技股份有限公司 © 2022-2023.