Ophiactis savignyi

Last updated

Ophiactis savignyi
Tiny in-a-sponge brittle stars (Ophiactis savignyi).jpg
Scientific classification OOjs UI icon edit-ltr.svg
Domain: Eukaryota
Kingdom: Animalia
Phylum: Echinodermata
Class: Ophiuroidea
Order: Ophiurida
Family: Ophiactidae
Genus: Ophiactis
Species:
O. savignyi
Binomial name
Ophiactis savignyi
(Müller & Troschel, 1842) [1]
Synonyms [1]
  • Ophiactis brocki de Loriol, 1893
  • Ophiactis conferta Koehler, 1905
  • Ophiactis incisa von Martens, 1870
  • Ophiactis krebsii Lütken, 1856
  • Ophiactis maculosa von Martens, 1870
  • Ophiactis reinhardti Lütken, 1859
  • Ophiactis reinhardtii Lütken, 1859
  • Ophiactis sexradia (Grube, 1857)
  • Ophiactis sixradia Lütken, 1853
  • Ophiactis versicolor H.L. Clark, 1939
  • Ophiactis virescens Lütken, 1856
  • Ophiolepis savignyi Müller & Troschel, 1842
  • Ophiolepis sexradia Grube, 1857

Ophiactis savignyi is a species of brittle star in the family Ophiactidae, commonly known as Savigny's brittle star or the little brittle star. It occurs in the tropical and subtropical parts of all the world's oceans and is thought to be the brittle star with the most widespread distribution. [2] It was first described by the German zoologists Johannes Peter Müller and Franz Hermann Troschel in 1842. The specific name honours the French zoologist Marie Jules César Savigny.

Contents

Description

The disc of O. savignyi is up to 5 millimetres (0.2 in) in diameter. The aboral (upper) surface is covered by large overlapping scales and bears a scattering of spines, especially round the edges of the disc. The (usually) six arms are long, slender and tapering, and are composed of many segments with joints between them. Each segment bears five or six thorny spines. The aboral surface of the disc is a pale greenish-brown colour and the large, triangular radial shields, close to the origins of the arms, are contrastingly darker. The oral (under) surface is cream-coloured. [2]

Distribution and habitat

O. savignyi has a near cosmopolitan distribution in warm seas. It is present in the western Indo-Pacific region, the eastern Pacific Ocean, and on both sides of the Atlantic Ocean. [3] The populations in the Pacific and the Atlantic Oceans were only united when the Panama Canal was cut across the Isthmus of Panama in 1914. [2]

This brittle star occurs from the intertidal zone down to about 500 metres (1,640 ft). It is found in all the zones of reefs, in mangrove habitats, in seagrass meadows, among seaweeds and in contaminated waters, and is often found living inside sponges, possibly as a commensal. [3]

Ecology

Ophiactis savignyi is a deposit feeder and a scavenger, feeding on the detritus that accumulates on the sea bed. It raises the tips of its arms to detect food particles, rolls any nutritious items into a ball and moves them to the mouth, manipulating them by means of the tube feet. Examination of the stomach contents showed the remains of bryozoans, foraminiferans and gastropod among the large quantities of detritus and grains of sand that this brittle star had ingested. [4]

Individual O. savignyi are either male or female, and they can reproduce either sexually or asexually. Sexual reproduction involves the liberation of sperm and eggs into the sea and the development and eventual settlement of planktonic larvae. Asexual reproduction is by fragmentation, each portion being the same sex as its parent. Small, immature individuals (disc diameter under 4 millimetres (0.16 in)) usually have six arms and can split themselves in two and then regenerate the missing parts of the disc and arms, often ending up with five arms. Most larger individuals have five arms and can also undergo fragmentation. The larger males do so more often than do the females, and this may account for the fact that there is an excess of males in the population. [5] After splitting, the brittle star may still be able to reproduce sexually but some fragments of the disc may have no gonads and thus be unable to spawn until regeneration is complete. [4] [6]

In Taiwan, mature gametes occur at any time from March to December, but most of the population of O. savignyi spawn during May and June. Fission takes place at any time of year but mostly occurs between July and December. Sampling the brittle stars throughout the year resulted in finding that 48% of the individuals inspected were in the process of regeneration. The sex ratio in this locality is twenty-four males for every one female. [7]

In Hawaii, this brittle star is often to be found living in association with a sponge such as Lissodendoryx schmidti (previously Damiriana hawaiiana). Up to twenty individuals can be found clumped together in cavities in the base of the sponge, the area being so filled with the slime secreted by the sponge that the brittle stars can hardly move their arms. These brittle stars often seem to have broken or partly regenerated arms. It is not clear how they enter the sponge, nor how they feed or reproduce. [8]

Related Research Articles

<span class="mw-page-title-main">Echinoderm</span> Exclusively marine phylum of animals with generally 5-point radial symmetry

An echinoderm is any deuterostomal animal of the phylum Echinodermata, which includes starfish, brittle stars, sea urchins, sand dollars and sea cucumbers, as well as the sessile sea lilies or "stone lilies". While bilaterally symmetrical as larvae, as adults echinoderms are recognisable by their usually five-pointed radial symmetry, and are found on the sea bed at every ocean depth from the intertidal zone to the abyssal zone. The phylum contains about 7,600 living species, making it the second-largest group of deuterostomes after the chordates, as well as the largest marine-only phylum. The first definitive echinoderms appeared near the start of the Cambrian.

<span class="mw-page-title-main">Starfish</span> Class of echinoderms, marine animal

Starfish or sea stars are star-shaped echinoderms belonging to the class Asteroidea. Common usage frequently finds these names being also applied to ophiuroids, which are correctly referred to as brittle stars or basket stars. Starfish are also known as asteroids due to being in the class Asteroidea. About 1,900 species of starfish live on the seabed in all the world's oceans, from warm, tropical zones to frigid, polar regions. They are found from the intertidal zone down to abyssal depths, at 6,000 m (20,000 ft) below the surface.

<span class="mw-page-title-main">Brittle star</span> Class of echinoderms closely related to starfish

Brittle stars, serpent stars, or ophiuroids are echinoderms in the class Ophiuroidea, closely related to starfish. They crawl across the sea floor using their flexible arms for locomotion. The ophiuroids generally have five long, slender, whip-like arms which may reach up to 60 cm (24 in) in length on the largest specimens.

<span class="mw-page-title-main">Echinasteridae</span> Family of starfishes

The Echinasteridae are a family of starfish in the monotypic order Spinulosida. The family includes eight genera and about 133 species found on the seabed in various habitats around the world.

Ophiocanops fugiens is a living species in the brittle star family Ophiocanopidae. Though once considered to be the only one living species in this brittle star family, recent research has brought to light three specimens of Ophiocanops that differ substantially from O. fugiens. It has been regarded as the most primitive brittle star, close to Paleozoic forms, though other authors have disagreed with the view. Classification of O. fugiens is highly argued. Ophiocanops is usually placed in the order Oegophiurida or regarded as a genus incertae sedis or even given its own subclass Oegophiuridea. Some recent data suggest its relationship to the extant family Ophiomyxidae.

<span class="mw-page-title-main">Asexual reproduction in starfish</span>

Asexual reproduction in starfish takes place by fission or through autotomy of arms. In fission, the central disc breaks into two pieces and each portion then regenerates the missing parts. In autotomy, an arm is shed with part of the central disc attached, which continues to live independently as a "comet", eventually growing a new set of arms. Fragmentation occurs on star fishes.

<i>Gorgonocephalus eucnemis</i> Species of brittle star

Gorgonocephalus eucnemis is a species of basket star in the class Ophiuroidea. It is found in circumpolar marine environments in the Northern Hemisphere. The scientific name for the genus comes from the Greek, gorgós meaning "dreadful" and cephalus meaning "head", and refers to the similarity between these basket stars and the Gorgon's head from Greek mythology with its writhing serpents for hair. The specific name eucnemis is from the Greek "good" and "boot".

<i>Ophiothrix suensoni</i> Species of brittle star

Ophiothrix suensoni, Suenson's brittle star or the sponge brittle star, is a species of marine invertebrate in the order Ophiurida. It is found in the Caribbean Sea and Gulf of Mexico. It is included in the subgenus Acanthophiothrix making its full scientific name Ophiothrix (Acanthophiothrix) suensoni.

<i>Amphiodia pulchella</i> Species of brittle star

Amphiodia pulchella is a species of brittle star belonging to Amphiuridae, a diverse family of the Ophiurida order.

<i>Ophiocoma scolopendrina</i> Species of brittle star

Ophiocoma scolopendrina is a species of brittle star belonging to the family Ophiocomidae. Restricted to life in the intertidal, they live in the Indo-Pacific. They can typically be found within crevices or beneath borders on intertidal reef platforms. Unlike other Ophiocoma brittle stars, they are known for their unique way of surface-film feeding, using their arms to sweep the sea surface and trap food. Regeneration of their arms are a vital component of their physiology, allowing them to efficiently surface-film feed. These stars also have the ability to reproduce throughout the year, and have been known to have symbiotic relationships with other organisms.

<i>Ophionereis reticulata</i> Species of brittle star

Ophionereis reticulata, the reticulated brittle star, is a brittle star in the family Ophionereididae. It is found in shallow parts of the western Atlantic, Caribbean Sea and Gulf of Mexico.

<i>Amphiura filiformis</i> Species of brittle star

Amphiura filiformis is a species of brittle star belonging to the family Amphiuridae. It is found on the seabed in the north east Atlantic Ocean and adjoining seas to a depth of 200 metres (660 ft). It digs itself a shallow burrow in the sand and waves its arms in the water above to suspension feed on plankton.

<i>Aquilonastra conandae</i> Species of starfish

Aquilonastra conandae is a species of starfish from the family Asterinidae found near the Mascarene Islands in the Indian Ocean. It is known for its asexual reproduction and is fissiparous. It is a small starfish, discrete and camouflaged, and occurs in coral reefs in the surf zone of large waves. The species was described in 2006 by Australian marine biologists P. Mark O'Loughlin and Francis Winston Edric Rowe, and gets its name from Chantal Conand.

<i>Ophiocoma echinata</i> Species of brittle star

Ophiocoma echinata, the spiny ophiocoma, is a species of brittle star belonging to the family Ophiocomidae. It is the type species of the genus Ophiocoma and is found in the tropical west Atlantic Ocean, the Caribbean Sea and the Gulf of Mexico.

<i>Ophiactis</i> Genus of brittle stars

Ophiactis is a genus of brittle stars (Ophiuroidea).

<i>Aquilonastra burtoni</i> Species of starfish

Aquilonastra burtoni is a species of small sea star from the family Asterinidae from the Red Sea which has colonised the eastern Mediterranean by Lessepsian migration through the Suez Canal, although the Mediterranean populations are clonal reproducing through fissiparous asexual reproduction. It was originally described in 1840 by the English zoologist and philatelist John Edward Gray.

<i>Ophiopholis aculeata</i> Species of brittle star

Ophiopholis aculeata, the crevice brittle star or daisy brittle star, is a species of brittle star in the family Ophiactidae. It has a circum-polar distribution and is found in the Arctic Ocean, the northern Atlantic Ocean and the northern Pacific.

<i>Ophiomusa</i> Genus of echinoderms

Ophiomusa is a genus of echinoderms belonging to the family Ophiolepididae that includes: sea urchins, sand dollars and sea cucumbers. Ophiurida are similar to starfish; they both have a central disc and five arms sprouting from the disc. One of the main distinguishing factors of an Ophiuroid is its arms; the arms of an Ophiurida are longer, thinner, and distinctly separated in comparison to those of a sea star.

<i>Ophiothela mirabilis</i> Species of echinoderm

Ophiothela mirabilis is a species of ophiuroid brittle star within the family Ophiotrichidae. O. mirabilis is an epizoic species which have a non-parasitic relationship with host sponges or gorgonians. Although native to the Pacific Ocean, it has invaded the Caribbean and southwestern Atlantic since late 2000. Many of its characteristics, including reproduction and diet, allow O. mirabilis opportunities to quickly propagate and spread through habitats.

References

  1. 1 2 Stöhr, Sabine (2015). Stöhr S, O'Hara T (eds.). "Ophiactis savignyi (Müller & Troschel, 1842)". World Ophiuroidea database. World Register of Marine Species . Retrieved 2015-07-11.
  2. 1 2 3 "Ophiactis savignyi: Savigny's Brittle Star". Encyclopedia of Life (EOL). Retrieved 2015-07-12.
  3. 1 2 Gondim, Anne I.; Alonso, Carmen; Dias, Thelma L.P.; Manso, Cynthia L.C.; Christoffersen, Martin L. (2013). "A taxonomic guide to the brittle-stars (Echinodermata, Ophiuroidea) from the State of Paraíba continental shelf, Northeastern Brazil". ZooKeys (307): 45–96. doi: 10.3897/zookeys.307.4673 . PMC   3689063 . PMID   23794923.
  4. 1 2 McKeton, Kara. "Little Brittle star (Ophiactis savignyi)". Marine Invertebrates of Bermuda. Retrieved 2015-07-12.
  5. Mladenov, P.V.; Emson, R.H. (1988). Density, size structure and reproductive characteristics of fissiparous brittle stars in algae and sponges: evidence for interpopulational variation in levels of sexual and asexual reproduction. Marine ecology progress series. Oldendorf, 42(2), 181-194.
  6. McGovern, Tamara N. (2002). "Sex-ratio bias and clonal reproduction in the brittle star Ophiactis savignyi". Evolution. 56 (3): 511–517. doi: 10.1111/j.0014-3820.2002.tb01362.x . PMID   11989681.
  7. Chao, S.-M.; Tsai, C.-C. (1995). "Reproduction and population dynamics of the fissiparous brittle star Ophiactis savignyi (Echinodermata: Ophiuroidea)". Marine Biology. 124 (1): 77–83. doi:10.1007/BF00349149.
  8. Keegan, Brendan F.; O'Connor, Brendan D.S. (1985). Echinodermata. CRC Press. pp. 604–. ISBN   978-90-6191-596-6.