Stelleroidea are stemless echinoderms that have a central disc from which five or more arms radiate. It includes the true starfish (Asteroidea), the brittle or serpent stars (Ophiuroidea), and the somasters (Somasteroidea). They appeared in Ordovician seas more than 450 million years ago. They are thought to be descended from unknown crinoids that lost their stalks but quickly developed arms for more efficient locomotion and feeding. The asteroids and ophiuroids have many living representatives; the somasters are nearly extinct.
True sea stars are classified in the Asteroidea, a group of echinoderms. Unlike the superficially similar brittle stars (Ophiuroidea), true sea stars have no sharp demarcation between arms and central body, and they move using tube feet rather than wriggling movements of the whole arms. True starfish and ophiuroids shared a common ancestor in the Ordovician; the fossil starfish pictured above is much more recent, coming from the Eocene of California.
Most sea stars are predators, feeding on sessile or slow-moving prey such as mollusks and barnacles. The aptly named crown-of-thorns starfish sea star specializes in corals, and may do considerable damage to coral reefs. Many, but not all, sea stars are able to turn a portion of their stomachs out through the mouth, and thus digest food outside of the body.
Ophiuroids are a large group (over 1600 species) of echinoderms that includes the brittle stars (Ophiurida) and basket stars (Euryalida). The more familiar Ophiurida, or brittle stars, usually have five arms and superficially resemble true sea stars (Asteroidea). However, brittle stars have long, flexible arms (hence the other common name for ophiuroids, "snake stars" and a central, armored, disk-shaped body that is clearly demarcated from the arms. Instead of crawling on hundreds of tube feet like sea star, brittle stars move fairly rapidly by wriggling their arms. These agile arms are supported by an internal skeleton of calcium carbonate plates that superficially look like vertebrae, and that are in fact called vertebral ossicles. These are moved by a system of muscles and linked together by ball-and-socket joints. The body and arms are also protected by calcium carbonate plates, and the arms generally bear delicate spines.
Basket stars (Euryalida) have a similar structure to brittle stars, although they are usually larger. However, their arms are very highly forked and branched, and even more flexible than those of brittle stars.
Ophiuroids can be found in most parts of the world, from the Arctic and Antarctic to the tropics. Ophiuroids are common in many shallow-water marine habitats, and include a few species which can adapt to brackish water, which is quite unusual for echinoderms. Ophiuroids are dominant in many parts of the deep sea, where in certain regions the bottom may swarm with brittle starts. Basket stars also tend to live in deeper water. Most ophiuroids are scavengers and detritus feeders, although they also prey on small live animals such as small crustaceans and worms. Some, in particular the basket stars, filter-feed on plankton with their arms.
Ophiuroids and asteroids probably shared a common ancestor. Early members of both appear in the early Ordovician, roughly 500 million years ago. Ophiuroids are not common fossils; as you might expect from the name "brittle star", ophiuroids rapidly fall to pieces after death, and are rarely preserved whole. At the top of this page is a specimen of Furcaster from the Hunsrück Slate of western Germany, a locality famous for its outstanding preservation of delicate fossils. Furcaster belongs to an extinct group of brittle stars, the Oegophuroidea. Instead of a single chain of "vertebrae" supporting the arms, oegophiuroids had two rows of supports alternating down each arm. This gave the arms a "zippered" appearance. Oegophiuroids went extinct in the Mississippian (late Carboniferous) period. The ophiuroid shown below has not been described, but is in the Ophiurida (true brittle stars) and is possibly referable to the genus Ophiura, which is still extant. This is a much later ophiuroid, from the late Cretaceous-age Moreno Formation, in the Panoche Hills of Fresno County, California.
Somasteroidea are an extinct subclass of asterozoan echinoderms (star-shaped echinoderms), known to have lived during the early Paleozoic (Spencer, 1951). Somasteroids first appear in the fossil record in the Early Ordovician (Tremadocian, ~510-493 Ma), just prior to the appearance of the other two asterozoan classes, Asteroidea (sea stars) and Ophiuroidea (brittle stars). While the asteroids and ophiuroids have subsequently undergone extensive radiations and represent the two most successful extant echinoderm classes, somasteroid forms do not appear in the fossil record after the late Devonian and are therefore thought to have been extinct since then (Spencer, 1951; Blake, 1982).
Somasteroids are flattened, fivefold radially symmetrical echinoderms that range in shape from that of a pentagon to that of a star with protruding arms. It appears that somasteroids were benthic marine animals that were filter- and/or detritus-feeders. Despite their relatively rigid arm structure, somasteroids are thought to have been somewhat mobile and able to scavenge along the ocean floor (Spencer, 1951).
Spencer's (1951) original organization of the early asterozoans was primarily based upon the activities of the arms with respect to feeding. While early asteroids had stout and muscular arms, adapted for a carnivorous diet of large food items, and early ophiuroids had long and narrow arms, adapted for feeding on small food particles present in or near the sea floor, the broad, undifferentiated, petaloid arms of somasteroids appeared to have had little or no role in feeding. More contemporary classification schemes of the asterozoans have relied upon the subsequent diversification of certain asterozoan arm morphological characteristics, such as the types and organization of arm skeletal elements. In the following description of somasteroid morphology, comparisons to asteroid and ophiuroid morphology will be made in an effort to signify some of the key defining characteristics.
Asterozoans, as described by Spencer (1951), have an appreciably flattened central body cavity from which five arms extend. As in asteroids, the arms and body of somasteroids are fully continuous. The arms and the disk-like body of ophiuroids, on the other hand, are clearly discontinuous. The two flat sides of asterozoans comprise the oral and aboral surfaces, of which the oral side is in contact with the substrate. A disjunct ossicular skeleton called a test covers both oral and aboral surfaces of asterozoans. Adjacent skeletal ossicles of the test are not rigidly fused as they are in crinoids and most echinoids, but are joined with connective and muscular tissues. The ossicular skeleton of somasteroids is often referred to as simple or undifferentiated when compared to that of asteroids and ophiuroids. Nevertheless, while the aboral test of somasteroids is composed of a single ossicle type (paxillae with tetraradiate bases), the oral test is significantly more complex.
The oral surface of each arm consists of two adjacent rows of recumbent ambulacral plates (ambulacrals). These ambulacrals, presumably involved in feeding, extend from the centrally located mouth to the tip of each arm. In asteroids, ophiuroids and most somasteroids, adjacent ambulacrals are arranged in a paired manner. In some early somasteroids, however, adjacent ambulacrals are alternately arranged. Each ambulacral gives rise to a transverse series of ossicles (metapinnules). These ossicles can occur as undifferentiated rod-like elements called virgals (found only in somasteroids), or as various differentiated elements including adambulacrals, intermediate ossicles, and marginal ossicles. When present in somasteroids and ophiuroids, adambulacrals are positioned laterally with respect to ambulacrals. In asteroids, however, adambulacrals are located underneath the ambulacrals. In addition, in asteroids the ambulacral plates are raised slightly off the surface upon which they sit, creating a space between the ambulacrals and the substrate. This space is often referred to as the ambulacral furrow or groove. Somasteroids and ophiuroids lack a permanent ambulacral furrow, although it appears that some derived somasteroids may have been able to create a temporary ambulacral furrow through muscular flexures.
Radial water vessels extend the length of each arm within a radial channel formed by the recumbent ambulacral plates and give rise to numerous tube feet (Figure 2). In somasteroids, the radial water vessel is often positioned at the oral-marginal junction of ambulacrals, as in asteroids, but can also be enclosed within the ambulacral plates, as in ophiuroids. Tube feet branching from the radial water vessels are seated in broad basins that, in some species, also give rise to ampulae that extend into the body cavity through ambulacral pores. The jaw ossicles of somasteroids are differentiated with small mouth angle plates, in contrast to those of asteroids that lack odontophores (McKnight, 1975). Buccal slits, which function primarily as respiratory structures in ophiuroids, may or may not have been present adjacent to the mouth frame in somasteroids.
Origin of Somasteroidea
Discussions addressing somasteroid origins have certainly been a major point of contention through the years primarily because the intermediate forms that gave rise to the somasteroids are lacking from the fossil record (Blake and Guensburg 1993; Blake, 1994). It seems most likely, however, that the somasteroids emerged from either a crinoid lineage (Fell, 1963; Mooi and David, 2000), or an edrioasteroid lineage (Paul and Smith, 1984; Smith 1988b).
Discussion of Phylogenetic Relationships
Informative evolutionary and phylogenetic analyses within Somasteroidea have been quite difficult because the examination and characterization of the group has been somewhat limited. What is known about the diversification of somasteroids, however, is primarily derived from work on three lower Ordovician families: Chinianasteridae (Tremadoc-Early Arenig), Villebrunasteridae (Tremadoc-Early Arenig), and Archegonasteridae (Late Arenig), as discussed by Nichols (1962), Fell (1963), and Blake (1982).
The Family Chinianasteridae is thought to include the most basal group of somasteroids based on the presence of undifferentiated virgals and robust ambulacrals, in addition to the absence of ampulae. The more derived Family Villebrunasteridae has differentiated virgals that include adambulacral, oral intermediate, and distinct marginal elements. Members of this group also have internal ampulae that provide a more direct connection between the body cavity and the environment. The most derived of these three families, the Archegonasteridae, represent the most thoroughly examined group of somasteroids. The Archegonasteridae have undergone a virgal reduction and have changed their body shape slightly from their predecessors to a more or less pentagonal outline with no interradial slits. In addition, Archegonasteridae specimens appear to have a more robust mouth frame than the more basal somasteroids and are often preserved with an ambulacral furrow. The latter two of these Archeogasteridae characteristics are also quite typical of asteroids and may very well have facilitated an adaptive change in feeding behavior from scavenging to predation.
Classification of Somasteroidea
The first organized classification of Somasteroidea was carried out by W. K. Spencer (1951). In his report, Spencer describes some of the earliest asteroid and ophiuroid specimens ever found. In addition, he describes fossils of a third asterozoan group, the somasteroids, which occur not only contemporaneously with, but also prior to all recognizable asteroid and ophiuroid fossil forms. These findings are suggestive of a scenario in which all asterozoans arose from ancient somasteroid forms.
Spencer (1951) assigned one order, Goniactinida, to the subclass Somasteroidea. Within this order he assigned two families, Chinianasteridae, including the genera Chinianaster (Tremadoc-Early Arenig) and Villebrunaster (Tremadoc-Early Arenig), and Archegonasteridae, composed of one genus, Archegonaster (Late Arenig). Subsequently, a seemingly extant somasteroid was identified by Fell (1962) in the Pacific off the coast of southern Mexico. This extant specimen, Platasterias latiradiata, was placed into a new somasteroid family, Platasteriidae (Fell, 1963a). The following year, Fell (1963b) reclassified the entire Asterozoa, and in so doing, removed Villebrunaster from the family Chinianasteridae and placed it in its own family Villebrunasteridae. Spencer and Wright (1966) added one more family, Archophiactinidae composed of three genera, Archophiactis (Late Ordovician), Stuertzurea (Silurian), and Lepidasterina (Late Devonian). McKnight (1975) then placed one more family, Helianthasteridae, previously an asteroid group, into Somasteroidea. The extant Platasterias latiradiata was subsequently reclassified by D. B. Blake (1982) and was placed in the Asteroidea. Platasteriidae was consequently removed from the somasteroids. This left five families and between 8-12 genera in the subclass Somasteroidea (Smith and Jell, 1990), as can be seen in the cladogram, based on Spencer and Wright (1966), McKnight (1975), and Blake (1982), shown above.
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