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Rathbunaster is a monospecific genus of sea stars belonging to the family Asteriidae.[1] The genus name was given by Fisher as a honorific of the starfish biologist Richard Rathbun of the Smithsonian Institution. He originally ranged this genus under the family Pycnopididae, synonymous with Asteriidae.
Rathbunaster californicusFisher, 1906,[2] common name California sun star, is a sea star belonging to the phylum Echinodermata and the class Asteroidea. It has a maximum size of about 45 centimeters in diameter[3]. The average weight of the star is 35 g, lives between sixty and a thousand meters in-depth, and lives on the muddy benthic substrate.[4] The surface of the star contains many spikes containing pincers. When something swims and lands on top of the California sun star, those pincers can grab onto the prey and capture the prey; then, the star will then grab the prey and eat it.[3]
Original description:[5]
It resembles closely Pycnopodia Stimpson, but differing in having a smaller disk, with the rays constricted at base and easily detachable. In the entire absence of rudimentary annular or calcareous ridges at the base of the ray, in the abortion of alternate supermarginal plates beyond the base of theray, and in the small widely spaced inferomarginals each bearing a slender spine; in the greater prominence of the adambulacral plates which are placed on the same level with the inferomarginals (and each with a single spine as in Pycnopodia); in the less crowded condition of the ambulacral ossicles.
The circular isolated plates on abactinal surface of rays are more numerous than in Pycnopodia and each bears a wreathed spine, whereas in Pycnopodia spines are rare on abactinal plates of arm. There are no large bivalved pedicellariae as in Pycnopodia. Tube-feet quadriserial except at extremity and base of ray where they are biserial. Ambulacral plates being less crowded, the tube feet are really intermediate in arrangement between the biserial and quadriserial type. Mouth plates are more prominent than in Pycnopodia and approach in form the type common to Brisingidae. The actinostome is wide, like the Brisingidae.
Rathbunaster californicus lives along the west coast of North America and ranges from southern California to southern Alaska. It is found in muddy substrates in the deep ocean/benthic environments. The star's distribution ranges from ninety nine to seven hundred sixty eight meters in depth.[6]
The California sun star has pentaradial symmetry. Pentaradial symmetry means if the star were cut into 5, each section would be the same. It has 15 arms, all centered around a central disk. In its larval stage, it exhibits bilateral symmetry. Instead, one surface is considered the oral and aboral surface. The oral surface consists of the mouth and tubular feet, while the aboral surface consists of the anus.[7]
The endoskeleton of the California sun star is made up of calcareous ossicles, which are covered in a thin layer of the ciliated tissue. The inside of the star is composed of the water vascular system, which is a complex system of fluid-filled canals within the star.[7]
The California sun star, like other members of Echinodermata, has tubular feet. These tubular feet are filled by the water vascular system. These tube feet serve the purpose of locomotion and help in feeding, gas exchange, and attachment to the surface. The tubular feet are also part of the nervous system. The nervous system in the California sun star is decentralized and has no cerebral ganglion. A lot of evidence shows that this nervous system can respond to touch, light, and water currents and shows the potential of having complex behavior.[7]
Rathbunaster californicus is a carnivore and a decomposer. It feeds on crustaceans, worms, detritus, and occasionally fish using its pincers on its aboral side. Due to the majority of its prey being benthic, a lot of sediment is found in the California sun stars stomach.[8] This sea star is known to be one of the main decomposers in the deep ocean and is known to be the main decomposer when a whale falls in the Monterey Canyon off the coast of California.[9] The stomach has strong digestive enzymes, and the California sun star is able to start digesting the organism before it even enters its digestive system. The digestive glands extend into the arms and are short.[3]
Rathbunaster californicus exhibits both asexual and sexual reproduction. If split in half, both halves will grow into two identical California sun stars. Sexually, the California sun star releases gametes into the water column. Gametes from male and female stars will meet in the water column, and the gamete is fertilized externally. During the embryonic stage, it is considered a deuterostome due to the anus forming from the blastopore, radial cleavage, and the archenteron developing from the coelom.[6]
The California sun star is a very important species in its ecosystems. It is one of the most abundant sea stars along the west coast of the United States and the most abundant star in the Monterey Canyon. The sea star plays multiple important ecological roles, such as it eats a variety of organisms and helping keep those organisms from overpopulating. The sea star also is a deep water decomposer and helps recycle nutrients and sequester carbon into the sediments.[4]
In the Monterey Canyon, Rathbunaster californicus has been found to be infected with a parasite. This parasite resembles Asterophila japonica, which is an endoparasitic gastropod. However, it is unknown. The unknown parasite could potentially be a new species of an endoparasitic gastropod. What is known is that this parasite is a member of Eulimidae. A main characteristic of Eulimidae is that they attach to the host permanently. Asterophila japonica attaches to the column of Rathbunaster californicus. The adult form of the parasite is visible as a lump in skin of Rathbunaster californicus.[4]
Rathbunaster is a monospecific genus of sea stars belonging to the family Asteriidae. The genus name was given by Fisher as a honorific of the starfish biologist Richard Rathbun of the Smithsonian Institution. He originally ranged this genus under the family Pycnopididae, synonymous with Asteriidae.
Rathbunaster californicusFisher, 1906, common name California sun star, is a sea star belonging to the phylum Echinodermata and the class Asteroidea. It has a maximum size of about 45 centimeters in diameter. The average weight of the star is 35 g, lives between sixty and a thousand meters in-depth, and lives on the muddy benthic substrate. The surface of the star contains many spikes containing pincers. When something swims and lands on top of the California sun star, those pincers can grab onto the prey and capture the prey; then, the star will then grab the prey and eat it.
Rathbunaster californicus est une espèce d'étoiles de mer de la famille des Asteriidae, la seule représentante du genre Rathbunaster.
C'est une grande étoile régulière munie de 12 à 20 bras longs, souples et robustes ; elle peut mesurer jusqu'à une quarantaine de centimètres de diamètre[2]. Sa face aborale est de couleur grisâtre à orange vif en passant par diverses teintes de rose, et apparaît rugueuse et granulée; L'épiderme est en fait couvert de gros pédicellaires.
On trouve cette étoile dans le Pacifique Nord-est, notamment sur la côte ouest des États-Unis[3]. On la trouve en grande profondeur, entre 100 et 768 m de fond[4].
Cette étoile a des habitudes omnivores opportuniste (oursins spatangoïdes, animaux benthiques plus lents qu'elles, etc.). Cependant, elle est aussi capable d'adopter un comportement de prédation active sur des animaux plus rapides, nageant en pleine eau[5] : elle lève ses bras couverts de puissants pédicellaires en forme de grosses mâchoires, qui saisissent l'épiderme de petits animaux (krill, crevettes, amphipodes, cnidaires, petits poissons...) et permettent à l'étoile de les piéger, puis de les attirer vers la bouche pour les dévorer[6].
L'espèce est parasitée par le mollusque Asterophila rathbunasteri[7].
Rathbunaster californicus est une espèce d'étoiles de mer de la famille des Asteriidae, la seule représentante du genre Rathbunaster.
Rathbunaster californicus is een zeester uit de familie Asteriidae.
De wetenschappelijke naam van de soort werd in 1906 gepubliceerd door Walter Kenrick Fisher.
Bronnen, noten en/of referenties
Wikimedia Commons'ta Rathbunaster californicus ile ilgili çoklu ortam belgeleri bulunur. 
Wikispecies'te Rathbunaster californicus ile ilgili detaylı taksonomi bilgileri bulunur. Rathbunaster californicus, Asteriidae familyasından, monotipik Rathbunaster cinsinde sınıflandırılan bir denizyıldızı türüdür. Pasifik Okyanusu'nun doğu kıyılarında derinsuda yaşar. On iki ila yirmi arasında kolu vardır. Cins adı Rathbunaster, Richard Rathbun'a ithafen verilmiştir.[3]
Rathbunaster californicus, Asteriidae familyasından, monotipik Rathbunaster cinsinde sınıflandırılan bir denizyıldızı türüdür. Pasifik Okyanusu'nun doğu kıyılarında derinsuda yaşar. On iki ila yirmi arasında kolu vardır. Cins adı Rathbunaster, Richard Rathbun'a ithafen verilmiştir.
