Rathbunaster is a monospecific genus of sea stars in the family Asteriidae.[1] The genus name was given by Walter Kenrick Fisher to honor the starfish biologist Richard Rathbun of the Smithsonian Institution. He originally ranged this genus under the family Pycnopididae, synonymous with Asteriidae.
| Rathbunaster | |
|---|---|
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| Original image of Rathbunaster californicus | |
Scientific classification 
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| Domain: | Eukaryota |
| Kingdom: | Animalia |
| Phylum: | Echinodermata |
| Class: | Asteroidea |
| Order: | Forcipulatida |
| Family: | Asteriidae |
| Genus: | Rathbunaster Fisher, 1906 |
| Species: | R. californicus
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| Binomial name | |
| Rathbunaster californicus Fisher, 1906
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The only species in the genus, Rathbunaster californicus,[2] common name California sun star, has a maximum size of about 45 centimeters in diameter[3] and an average weight of 35 g. It lives on muddy benthic substrates between 60 and 1,000 m below the surface.[4] it is covered in spikes with pincers that are used to capture prey for consumption.[3]
Description
editOriginal description:[5]
It resembles closely Pycnopodia Stimpson, but differing in having a smaller disk, with the rays constricted at the 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 the ray, 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.
Distribution
editRathbunaster californicus lives along the west coast of North America from southern California to southern Alaska. It is found in muddy substrates in deep ocean/benthic environments and has been found at depths of 60 and 1,000 m below the surface off of California[4] and depths from 99 to 768 m off the coast from the Puget Sound to Alaska.[6]
Anatomy and body plan
edit
Rathbunaster californicus has pentaradial symmetry. It has 8–20 arms, all centered around a central disk.[7] In its larval stage, it exhibits bilateral symmetry. Instead, one surface is considered the oral surface and the other the aboral surface. The oral surface consists of the mouth and tubular feet, while the aboral surface consists of the anus.[8][failed verification]
The endoskeleton of R. californicus is made up of calcareous ossicles, which are covered in a thin layer of the ciliated tissue. Inside there is a water vascular system, a complex system of fluid-filled canals.[8]
Rathbunaster californicus, like other members of Echinodermata, has tubular feet. These feet are filled by the water vascular system. They are used for locomotion and help in feeding, gas exchange, and attachment to the surface. They are also part of the nervous system, which is decentralized and has no cerebral ganglion. The nervous system can respond to touch, light, and water currents and shows the potential of having complex behavior.[8]
Diet and digestion
editRathbunaster californicus is a carnivore and decomposer. It feeds on crustaceans, worms, detritus, and fish using pincers on its aboral side. Because the majority of its prey is benthic, sediment is found in the stomach.[9] One of the main decomposers in the deep ocean, it has been observed assisting in the decomposition of whale carcasses in the Monterey Canyon.[10] The stomach has strong digestive enzymes, and R. californicus can start digesting food before it even enters its digestive system. The short digestive glands extend into the arms.[3]
Reproduction
editRathbunaster californicus exhibits both asexual and sexual reproduction. If split in half, both halves will grow into two identical organism. Sexually, R. californicus releases gametes into the water column. Male and female gametes 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]
Ecological impact
editRathbunaster californicus 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. It plays multiple important ecological roles, eating a variety of organisms and controlling populations of those species. It is also a deep water decomposer and helps recycle nutrients and sequester carbon into sediments.[4]
Parasite
editIn the Monterey Canyon, R. californicus has been found infected with a parasite thought to be Asterophila japonica, an endoparasitic gastropod. The unknown parasite could potentially be a new species of endoparasitic gastropod. The parasite, a member of Eulimidae, attaches to the column of R.californicus. The adult form of the parasite is visible as a lump in the skin.[4]
References
edit- ^ Mah, C.L. (2022). World Asteroidea Database. Rathbunaster Fisher, 1906. Accessed through: World Register of Marine Species at: https://www.marinespecies.org/aphia.php?p=taxdetails&id=254843 on 2022-04-25
- ^ "WoRMS - World Register of Marine Species - Rathbunaster californicus Fisher, 1906". www.marinespecies.org. Retrieved 2022-04-22.
- ^ a b c "California sun star". MBARI. 2020-12-21. Retrieved 2022-04-21.
- ^ a b c d Lewis, Lynn Morgan (1992). "Habitat Use, Diet, and Parasitism of the Seastar Rathbunaster Californicus Fisher from the Monterey Submarine Canyon". ProQuest Dissertations Publishing.
- ^ Fisher, W.K. (1906). New starfishes from the Pacific Coast of North America. Proceedings of the Washington Academy of Sciences. 8: 111-139
- ^ a b "Rathbunaster californicus, California sun star". www.sealifebase.ca. Retrieved 2022-04-22.
- ^ Simons, Eric (2019-10-15). "Science Explainer | Deep-Sea Sea Stars on the Hunt". Bay Nature. Retrieved 2023-10-11.
- ^ a b c Fau, Marine (2020). "Comparative Anatomy and Phylogeny of the Forcipulatacea (Echinodermata: Asteroidea): Insights from Ossicle Morphology". Zoological Journal of the Linnean Society. 189 (3): 921–952. doi:10.1093/zoolinnean/zlz127.
- ^ Lauerman, Lynn M (1988). "Diet and Feeding Behavior of the Deep-Water Sea Star Rathbunaster Californicus (Fisher) in the Monterey Submarine Canyon". Bulletin of Marine Science: 520–530.
- ^ Lundsten, Lonny; Schlining, Kyra L.; Frasier, Kaitlin; Johnson, Shannon B.; Kuhnz, Linda A.; Harvey, Julio B. J.; Clague, Gillian; Vrijenhoek, Robert C. (2010-12-01). "Time-series analysis of six whale-fall communities in Monterey Canyon, California, USA". Deep Sea Research Part I: Oceanographic Research Papers. 57 (12): 1573–1584. Bibcode:2010DSRI...57.1573L. doi:10.1016/j.dsr.2010.09.003. ISSN 0967-0637.