Rathbunaster

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Rathbunaster
Rathbunaster californicus 001.png
Original image of Rathbunaster californicus
Scientific classification OOjs UI icon edit-ltr.svg
Domain: Eukaryota
Kingdom: Animalia
Phylum: Echinodermata
Class: Asteroidea
Order: Forcipulatida
Family: Asteriidae
Genus: Rathbunaster
Fisher, 1906
Type species
Rathbunaster californicus
Fisher, 1906

Rathbunaster is a monospecific genus of sea stars belonging to the family Asteriidae. [1] The genus name was given by Walter Kenrick 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.

Contents

Rathbunaster californicus, [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 one thousand meters in-depth, and lives on the muddy benthic substrate. [4] The sea star's surface is covered in spikes with pincers, used to grab and capture prey for consumption. [3]

Description

Original 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 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.

Distribution

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]

Anatomy and body plan

Rathbunaster californicus with arms extended Olympic Coast National Marine Sanctuary 2010 Pycnopodia helianthoides.jpg
Rathbunaster californicus with arms extended

The California sun star 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 and 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 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. [8]

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. [8]

Diet and digestion

Rathbunaster californicus is a carnivore and decomposer. It feeds on crustaceans, worms, detritus, and fish using pincers on its aboral side. Due to the majority of its prey being benthic, sediment is found in the California sun star's stomach. [9] One of the main decomposers in the deep ocean, the California sun star, has been observed assisting in the decomposition of whale carcasses in the Monterey Canyon. [10] 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 short digestive glands extend into the arms. [3]

Reproduction

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]

Ecological impact

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]

Parasite

In the Monterey Canyon, Rathbunaster 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 Rathbunaster californicus. The adult form of the parasite is visible as a lump in the skin of Rathbunaster californicus. [4]

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References

  1. 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
  2. "WoRMS - World Register of Marine Species - Rathbunaster californicus Fisher, 1906". www.marinespecies.org. Retrieved 2022-04-22.
  3. 1 2 3 "California sun star". MBARI. 2020-12-21. Retrieved 2022-04-21.
  4. 1 2 3 Lewis, Lynn Morgan (1992). "Habitat Use, Diet, and Parasitism of the Seastar Rathbunaster Californicus Fisher from the Monterey Submarine Canyon". ProQuest Dissertations Publishing.
  5. Fisher, W.K. (1906). New starfishes from the Pacific Coast of North America. Proceedings of the Washington Academy of Sciences. 8: 111-139
  6. 1 2 "Rathbunaster californicus, California sun star". www.sealifebase.ca. Retrieved 2022-04-22.
  7. Simons, Eric (2019-10-15). "Science Explainer | Deep-Sea Sea Stars on the Hunt". Bay Nature. Retrieved 2023-10-11.
  8. 1 2 3 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 .
  9. 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.
  10. 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.

Bibliography