Ophiocoma scolopendrina

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Ophiocoma scolopendrina
Ophiocomidae - Ophiocoma scolopendrina.jpg
Ophiocoma scolopendrina at Sharm El Sheik, Red Sea
Scientific classification Red Pencil Icon.png
Kingdom: Animalia
Phylum: Echinodermata
Class: Ophiuroidea
Order: Ophiacanthida
Family: Ophiocomidae
Genus: Ophiocoma
Species:
O. scolopendrina
Binomial name
Ophiocoma scolopendrina
(Lamarck, 1816)
Synonyms
  • Ophiocoma alternans von Martens, 1870
  • Ophiocoma lubrica Koehler, 1898
  • Ophiocoma molaris Lyman, 1862
  • Ophiocoma variabilis Grube, 1857
  • Ophiura scolopendrina Lamarck, 1816

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. [1] 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. [2] Regeneration of their arms are a vital component of their physiology, allowing them to efficiently surface-film feed. [3] These stars also have the ability to reproduce throughout the year, and have been known to have symbiotic relationships with other organisms. [4]

Contents

Description

Ophiocoma scolopendrina, as other brittle stars, have long, thin arms emanating from a small, disk-shaped body and are about the size of an outstretched human hand. They belong to the phylum of echinoderms, which includes sea urchins, sea cucumbers, and sea stars. Dorsal disc and dorsal arm plates vary from variegated black to pale brown. They are irregularly banded. O. scolopendrina can reach a length of about 13cm, while the disc diameter can reach up to 25mm. [5] The star's sexes can be identified by checking slits between the arms, which expose the white male spermaries and red female ovaries. [6]

Distribution and habitat

Ophiocoma scolopendrina can be found in the Red Sea, [7] the tropical Indo-Pacific region, Taiwan, Eastern Africa, Southeastern Polynesia, the Marshall Islands, and Madagascar. Their typical density is about 20 individuals per 1m². [3]

These brittle stars are present in crevices [8] and under boulders of intertidal reef platforms in the upper and middle eulittoral. They have also been seen underneath coral rubble. They typically hide amongst concealing vegetation during surface-film feeding. They live primarily in areas with shallow water strictly in the intertidal [1] and are often observed sweeping their arms over sand or coral substrata. [2]

Feeding

Behavior

Ophiocoma scolopendrina in its natural habitat Ophiocoma scolopendrina.jpg
Ophiocoma scolopendrina in its natural habitat

When feeding, O. scolopendrina changes its location depending on tide positionality. Stars have been observed to be nearly entirely concealed at high tide, and expose themselves progressively as the tide becomes lower. [2]

Unlike other brittle star species [9] , these stars have evolved an adaptation that lets them participate in surface-film feeding during both low and flooding tides. [2] This adaptation allows them to consume neuston and detrital particles and film that are found suspended on the surface of sea water.

During feeding, O. scolopendrina becomes fully exposed and remains attached to the ground by anchoring an arm to a substratum or piece of vegetation. Occasionally, they may also climb vegetation to gain better feeding positionality. The brittle star then utilizes two to four arms to sweep the sea surface, using its arms' ventral sides to trap suspended objects into mucous-covered spines. The food is then transferred to the mouth once the spines have been cleaned by tube feet. [10]

Outside of flooding tide, these brittle stars simply participate in microphagous suspension and deposit-feeding, behavior that is common for other Ophiocoma species. [10] During these types of feedings, arms are extended and food is caught from the water column into their mucous-covered spines during this process. This has typically been observed after a high tide.

The unusual feeding pattern observed in Ophiocoma scolopendrina has been attributed to a variety of influences, including changes in tidal patterns, the presence of predation, and food availability. [2]

Reproduction

Ovarian substances have been noted to induce male spawn. [8] Adult female stars each contain an estimated 12 * 10⁵ premature oocytes and it is believed that all adult O. scolopendrina produce gametes throughout the remainder of their lives. They consistently produce gametes at all studied ages. [11] O. scolopendrina reproduce continuously throughout the year, as once gametes are available in the gonads, allowing them to spawn regardless of season.

Ophiocoma scolopendrina have planktonic planktotrophic larvae [5] and have been observed to spawn in large numbers.

Regeneration

Ophiocoma scolopendrina with arms of different lengths OFIURA ili ZMEEKhVOSTKA. Schlangensterne (Ophiuroidea),Stachelhauter (Echinodermata) 2H1A5193WI.jpg
Ophiocoma scolopendrina with arms of different lengths

Similar to other types of brittle stars, O. scolopendrina has the ability to regenerate its arms. [3] Stars may be injured by a variety of means, from general aggression and predation to the intense waves of their ecosystems. To account for this loss, stars regenerate these damaged portions of their arms, investing incredible amounts of energy as a means to survive for a longer amount of time. Regeneration, in turn, allows for the recuperation in functionality and strength in that arm. This adaptation has become vital in allowing brittle stars to survive even the harshest of environments. [12]

Compared to other brittle stars, O. scolopendrina does not lose parts of its arms as rapidly as expected. Arms are important sources of feeding and have been noted to be used as a means of quick predator evasion. Since arms are used for both food capture and locomotion, O. scolopendrina are more hesitant to expose their arms to harmful situations. [12]

Given O. scolopendrina's positionality in its ecosystem, breakage has typically been mainly observed in the top third of the arm. [3] Since these types of stars spend a majority of their time hidden in crevices, only the tips of their arms suffer the most damage. In many cases, these arms remain functional, however, as the majority of the arm is not exceedingly damaged. Arms that are used for anchorage within crevices are those least likely to be lost as they are not frequently exposed to the dangers of the intertidal. Those that are out, whether it be for feeding or general sweeping, have been noted to be the arms most affected. [3]

Multiple arm breakages have also been seen to occur in O. scolopendrina. [3] As one arm may be damaged by a predator or ecological force, other arms must take its place as the most frequently used, causing them to suffer more harm than otherwise. Those that dwell in poor habitats are oftentimes more vulnerable to the forces of nature and are subject to consistent damage to their bodies. The average rate of regeneration is about 0.4 mm/day. [3]

Heterospecific symbiosis

Adult Ophiocoma scolopendrina have a heterospecific symbiotic relationship with juveniles of Ophiomastix annulosa in the intertidal zone of Okinawa, Japan. [4] In this region, younger O. annulosa have been observed to attach to the bursae of the living O. scolopendrina host. It is thought that O. annulosa's hooked terminal spines may be advantageous in remaining attached to the host star, as they are difficult to dislodge. Symbionts typically switch hosts as they become larger, switching between new O. scolopendrina hosts as their size increases. [4] The relationship between these stars has largely been considered a form of brood parasitism, as O. annulosa young are, in a sense, cared for by the O. scolopendrina adults and there is no physical damage to the host organism. [4]

Related Research Articles

Echinoderm Exclusively marine phylum of animals with generally 5-point radial symmetry

An echinoderm is any member of the phylum Echinodermata of marine animals. The adults are recognizable by their radial symmetry, and include starfish, sea urchins, sand dollars, and sea cucumbers, as well as the sea lilies or "stone lilies". Adult echinoderms are found on the sea bed at every ocean depth, from the intertidal zone to the abyssal zone. The phylum contains about 7000 living species, making it the second-largest grouping of deuterostomes, after the chordates. Echinoderms are the largest phylum that has no freshwater or terrestrial members.

Starfish 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 occur on the seabed in all the world's oceans, from the tropics to frigid polar waters. They are found from the intertidal zone down to abyssal depths, 6,000 m (20,000 ft) below the surface.

Brittle star Class of brittle stars

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. From New Latin ophiurus, from Ancient Greek ὄφις + οὐρά.

<i>Protoreaster nodosus</i> Species of starfish

Protoreaster nodosus, commonly known as the horned sea star or chocolate chip sea star, is a species of sea star found in the warm, shallow waters of the Indo-Pacific region. They are sometimes seen in the marine aquarium trade.

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.

<i>Ophiura ophiura</i> Species of brittle star

Ophiura ophiura or the serpent star is a species of brittle star in the order Ophiurida. It is typically found on coastal seabeds around northwestern Europe.

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>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>Astroboa nuda</i> Species of brittle star

Astroboa nuda is a type of basket star from Gorgonocephalidae family. Its large arms are highly branched. It inhabits reef slopes exposed to current in diverse places such as the Red Sea and New Caledonia. During the day it coils into a tight ball. At night it spreads arms to form a basket to feed on plankton. They are part of the class Ophiuroidea, which is the largest class of echinoderms. The name Ophiuroidea comes from the roots, ophis, meaning snake and oura, which means tail, referring to the thin, spiraling shape of the basket stars’ arms.

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

Gorgonocephalus arcticus is a species of basket star in the class Ophiuroidea. The genus name comes from the Greek, gorgós meaning "dreaded" and cephalus meaning "head", and refers to the similarity between these echinoids and the Gorgon's head from Greek myth with its coiled serpents for hair.

<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 savignyi</i> Species of brittle star

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. 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.

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

Ophiothrix angulata, the angular brittle star, is a species of marine invertebrate in the order Ophiurida. It is found in the warm waters of the western Atlantic Ocean, the Caribbean Sea and the Gulf of Mexico.

<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>Astrobrachion adhaerens</i> Species of brittle star

Astrobrachion adhaerens is a basket star in the Euryalidae family. Along with A. constrictum, it is one of only two species in the genus Astrobrachion. Both species live in association with soft corals in moderately deep water. It is endemic to the west, north and east coasts of Australia, the Kermadec Islands and Lord Howe Island.

<i>Acrocnida</i> Genus of echinoderms

Acrocnida is a genus of brittle stars in the family Amphiuridae. The genus contains three members: Acrocnida brachiata, Acrocnida semisquamata, and Acrocnida spatulispina. There has also been observed hybridization between both Acrocnida brachiata and Acrocnida spatulispina. It is a fairly common genus, usually found along the coasts of Northwestern Europe, but with some species like semisquamata appearing around West Africa. Members of this genus primarily prefer intertidal and sub-tidal habitats, and they are they are less likely to be found in intertidal areas by comparison. This genus was not officially classified until 1926, by T. Gislén. One study found that due to the increased calcification that Acrocnida brachiata causes could be a potential source of Carbon Dioxide for not only the warm, shallow environments they live in, but also for the atmosphere.

<i>Ophiocomella alexandri</i> Species of brittle star

Ophiocomella alexandri, known as Alexander's spiny brittle star or banded brittle star, is a species of marine brittle star. It was first described to science by Theodore Lyman in 1860. Lyman states in his description that the animal is named for his friend, Alexander E. R. Agassiz, the son of Lyman's mentor, Louis Agassiz.

<i>Ophiomastix wendtii</i> Species of brittle star

Ophiomastix wendtii, also known by its common name, the red ophiocoma, and formerly as Ophiocoma wendtii, is a species of brittle stars that inhabits coral reefs from Bermuda to Brazil, primarily in the Caribbean sea. It is known for its advanced compound eyes and club-like spines along its arms. These brittle stars have long, thin arms emanating from a small, disk-shaped body, and are about the size of an outstretched human hand.

References

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