Asterozoa

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Asterozoa
Temporal range: 488.2–0  Ma
Seeing Stars 52868364563.jpg
A brittle star on a starfish
Scientific classification OOjs UI icon edit-ltr.svg
Domain: Eukaryota
Kingdom: Animalia
Phylum: Echinodermata
Subphylum: Asterozoa
von Zittel, 1895 [1]
Classes [2]
Synonyms
  • Stelleroidea Lamarck, 1816 [nom. transl. et correct. Gregory, 1900 (pro les Stellerides Lamarck, 1816)] [3]

The Asterozoa are a subphylum in the phylum Echinodermata, within the Eleutherozoa. Characteristics include a star-shaped body and radially divergent axes of symmetry. The subphylum includes the classes Asteroidea (the starfish or sea stars), Ophiuroidea (the brittle stars and basket stars), Somasteroidea (early asterozoans from which the other classes most likely evolved), and Stenuroidea (early asterozoans with unclear relationships to extant classes). [2] A fifth class, Concentricycloidea, was proposed for the unusual genus Xyloplax (sea daisies), [4] but was later demoted to the status of infraclass as the sister of Neoasteroidea within the asteroidean sublcass Ambuloasteroidea. [5]

Contents

Taxonomy

Asterozoa was originally proposed in the late 1800s, but was not used in F.A. Bather's two-subphylum echinoderm taxonomy in 1900. However, it was adopted as part of a four-subphylum taxonomy by the Treatise on Invertebrate Paleontology in 1966. [6]

Asterozoa is generally thought to be a monophyletic clade; its sister group within Eleutherozoa is Echinozoa. [7] The external affinities of Asterozoa are unclear. It has been proposed to derive from either the Edrioasteroidea or the Crinoidea, but no form of either proposal has gained wide acceptance due to the lack of any transitional fossils. [8]

Distinguishing the classes

Villebrunaster-virgals.png
Villebrunaster thorali (Somasteroidea)
Chinianaster-virgals.png
Chiniaster (Somasteroidea)
Stuertzaster-virgals.png
Stuertzaster (Stenuroidea)
Differences in virgals between somasteroids and stenuroids; note that in somasteroids the number of virgals per ambulacral varies based on the width of the arm, while the number of virgals (labeled as inner and outer laterals) in stenuroids is the same along the entire length of the arm.

Somasteroids and stenuroids are distinguished from each other and from the extant asteroids and ophiuroids by the arrangements of a specific type of ossicle known as virgals: Somasteroids possess a varying number of virgals per series extending laterally from the ambulacral ossicles, with at least some series exceeding three virgals. Stenuroids possess series of exactly two (or rarely three or four) virgals for each ambulacral ossicle, with other ossicular specializations. Asteroid and ophiuroid virgal series are each reduced to a single ossicle in addition to their more obvious morphological differences. [9]

Somasteroidea

Most authors consider Somasteroidea to be the basal stock from which the other three classes evolved., [10] [11] but an argument in favor of monophyly and a position closer to stenuroids and ophiuroids than to asteroids has also been made. [12]

Somasteroids are "more or less petaloid," with arm shape reflecting virgal series lengths. [13] Somasteroids have been described as being more rigid in shape than derived asterozoans, although this apparent structure could be exaggerated by tissue changes at the time of death. [14] S

Stenuroidea

Stenuroids were initially seen as early ophiuroids [15] before being promoted to class level, but their evaluation is challenging due to wide variations in morphologies. Some stenuroids appear closer to asteroids, others to ophiuroids, and others do not closely resemble either extant class. [16] A recent examination of Stenuroidea found it to be monophyletic, but allowed that (as with other asterozoan classes), paraphyly or polyphyly could not be entirely ruled out. [17] Other authors have considered that Stenuroidea is likely paraphyletic. [2]

Asteroidea

Asteroids have a permanently vaulted ambulacral furrow down the center of the underside of each arm. They use their tube feet for locomotion and (in many species) to pry open shells and access food. [18] Their arms touch at the base, and there is no clear border between the arms and the central disc. [19]

Ophiuroidea

Ophiuroid arms have evolved joints within their arms allowing lateral, snake-like movements for locomotion, while the tube feet are significantly reduced. [18] The central disc is clearly marked off from the arms. [19]

Related Research Articles

<span class="mw-page-title-main">Echinoderm</span> Marine phylum of animals often with radial symmetry

An echinoderm is any 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">Crinoid</span> Class of echinoderms

Crinoids are marine invertebrates that make up the class Crinoidea. Crinoids that remain attached to the sea floor by a stalk in their adult form are commonly called sea lilies, while the unstalked forms, called feather stars or comatulids, are members of the largest crinoid order, Comatulida. Crinoids are echinoderms in the phylum Echinodermata, which also includes the starfish, brittle stars, sea urchins and sea cucumbers. They live in both shallow water and in depths of over 9,000 metres (30,000 ft).

<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.

The water vascular system is a hydraulic system used by echinoderms, such as sea stars and sea urchins, for locomotion, food and waste transportation, and respiration. The system is composed of canals connecting numerous tube feet. Echinoderms move by alternately contracting muscles that force water into the tube feet, causing them to extend and push against the ground, then relaxing to allow the feet to retract.

<span class="mw-page-title-main">Stelleroidea</span> Class of marine invertebrates

Stelleroidea is a junior synonym of Asterozoa.

<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">Crinozoa</span> Subphylum of marine invertebrates

Crinozoa is a subphylum of mostly sessile echinoderms, of which the crinoids, or sea lilies and feather stars, are the only extant members. Crinozoans have an extremely extensive fossil history.

<span class="mw-page-title-main">Taxonomy of commonly fossilised invertebrates</span>

The taxonomy of commonly fossilized invertebrates combines both traditional and modern paleozoological terminology. This article compiles various invertebrate taxa in the fossil record, ranging from protists to arthropods. This includes groups that are significant in paleontological contexts, abundant in the fossil record, or have a high proportion of extinct species. Special notations are explained below:

<span class="mw-page-title-main">Eleutherozoa</span> Clade of echinoderms

Eleutherozoa is a subphylum of echinoderms. They are mobile animals with the mouth directed towards the substrate. They usually have a madreporite, tube feet, and moveable spines of some sort. It includes all living echinoderms except for crinoids. The monophyly of Eleutherozoa has been proven sufficiently well to be considered "uncontroversial."

<span class="mw-page-title-main">Deuterostome</span> Superphylum of bilateral animals

Deuterostomes are bilaterian animals of the superphylum Deuterostomia, typically characterized by their anus forming before the mouth during embryonic development. Deuterostomia is further divided into four phyla: Chordata, Echinodermata, Hemichordata, and the extinct Vetulicolia known from Cambrian fossils. The extinct clade Cambroernida is thought to be a member of Deuterostomia.

<span class="mw-page-title-main">Forcipulatida</span> Order of sea stars

The Forcipulatida are an order of sea stars, containing three families and 49 genera.

<i>Camptostroma</i> Extinct genus of marine invertebrates

Camptostroma roddyi is an extinct echinoderm from the Bonnia-Olenellus Zone of the Early Cambrian Kinzers Formation near York and Lancaster, Southeastern Pennsylvania. It is the only known species in the genus Camptostroma, as other species referred to this genus "do not appear to be cogeneric."

<span class="mw-page-title-main">Brisingida</span> Order of starfishes

The Brisingids are deep-sea-dwelling starfish in the order Brisingida.

<span class="mw-page-title-main">Homalozoa</span> Extinct historic group of marine invertebrates

Homalozoa is an obsolete extinct subphylum of Paleozoic era echinoderms, prehistoric marine invertebrates. They are also referred to as carpoids.

Pelmatozoa was once a clade of Phylum Echinodermata. It included stalked and sedentary echinoderms. The main class of Pelmatozoa were the Crinoidea which includes sea lily and feather star.

Xyloplax medusiformis is a sea daisy, a member of an unusual group of marine taxa belonging to the phylum Echinodermata. It is found at bathyal depths in waters around New Zealand. It was first described in 1986 by Baker, Rowe and Clark and is the type taxon of the genus Xyloplax. Its generic name derives from the Greek "xylo" meaning wood and its specific name was chosen because its morphology superficially resembles that of a cnidarian medusa.

<span class="mw-page-title-main">Ossicle (echinoderm)</span> Small calcium elements embedded in the dermis of the body wall of echinoderms

Ossicles are small calcareous elements embedded in the dermis of the body wall of echinoderms. They form part of the endoskeleton and provide rigidity and protection. They are found in different forms and arrangements in sea urchins, starfish, brittle stars, sea cucumbers, and crinoids. The ossicles and spines are the only parts of the animal likely to be fossilized after an echinoderm dies.

<span class="mw-page-title-main">Somasteroidea</span> Extinct order of asterozoan echinoderms

The Somasteroidea, or Stomasteroidea, is an extinct order of asterozoan echinoderms first defined in 1951 by W. K. Spencer. Their first appearance in the fossil record was in the Early Ordovician (Tremadocian) and they had become extinct by the Late Devonian (Famennian). They are similar to the asteroids in that their bodies are flattened dorsoventrally and they have five petaloid arms with broad bases. The ambulacral plates in somasteroids are simple and unspecialized, and the arms were thought to be not flexible and were unable to assist in feeding, but the oral mouth parts were more complex.

Helen Elizabeth Shearburn Rotman was a New Zealand expert on echinoderms, specifically starfish.

<i>Villebrunaster</i> Extinct genus of echinoderms

Villebrunaster is an extinct genus of starfish-like animal belonging to Asterozoa that lived around 480 million years ago during Early Ordovician Period in modern-day southern France and Morocco. As of 2022, it contains two species, namely V. thorali and V. fezouataensis. V. thorali was described in 1951 and V. fezouataensis was described in 2021. Villebrunaster represents one of the oldest members of asterozoans, and perhaps, according to a description in 2021, the earliest divergent stem-group of Asterozoa.

References

Works cited

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  • Blake, Daniel B.; Guensburg, Thomas E. (2015). "The class Somasteroidea (Echinodermata, Asterozoa): morphology and occurrence". Journal of Paleontology. 89 (3): 465–486. doi:10.1017/jpa.2015.22.
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  • Spencer, W. K.; Wright, C. W. (1966). "Asterozoans". In Moore; Raymond C. (eds.). Treatise on Invertebrate Paleontology, Part U: Echinodermata 3. Vol. 1. University of Kansas Press. pp. U5–U107. Retrieved 28 October 2024.