Amphiodia occidentalis
Scientific classification Edit this classification
Domain: Eukaryota
Kingdom: Animalia
Phylum: Echinodermata
Class: Ophiuroidea
Order: Ophiurida
Family: Amphiuridae
Genus: Amphiodia
Species:
A. occidentalis
Binomial name
Amphiodia occidentalis
(Lyman, 1860)[1]

Amphiodia occidentalis, the long-armed brittle star, is a species of brittle star belonging to the family Amphiuridae. It is found in the Eastern Pacific coast from Alaska to USA, [2] often on the seafloor within intertidal and subtidal zones. Within these areas, it is often found buried a few centimeters under the sand with 2 or 3 arms extending through the surface.[3]

Description

Amphiodia occidentalis exhibit pentaradial symmetry characteristic of brittle stars. They contain a flat disc body which can measure up to 11 mm in diameter [4] that contains their organs.[5] Five long, segmented arms at least eight times the diameter of the disc extend from the body which are covered in flattened spines [6] and tube feet.[7]

Additionally, they have a calcium carbonate endoskeleton composed of calcareous ossicles.[7] Their central nervous system is highly metameric with the same pattern of peripheral nerves repeated in each arm.[8]

Locomotion

Instead of using their tube feet for locomotion, Amphiodia occidentalis and several other brittle star species use their arms to crawl along the substrate.[9]

Despite their radial symmetry, they move using bilaterally symmetrical locomotion.[9] Since they lack a locomotor anterior, they achieve this type of locomotion by employing two techniques: rowing and reverse rowing.[9] The most common technique is the rowing technique, in which the center limb is in the front, towards the direction of movement, with the other limbs helping to move in the direction of the center limb. In reverse rowing, the center limb drags in the back, the opposite direction of movement, as the other limbs propel away from the center limb. In both techniques, the designated right and left forelimbs are highly synchronized while the hind limbs present greater variability.[7] When changing directions, the disc does not rotate. Depending on the new direction, they designate the appropriate limb as the center limb and designate new identities to the other limbs corresponding to their position to the central limb. Rowing or reverse rowing is then utilized to move according to the new center limb.[9]

Diet

Amphiodia occidentalis are facultative detritivores, mainly eating detritus on the seafloor [5][3] but can feed in other ways. By using their tube feet to catch food particles, they also engage in suspension feeding.[7]

Reproduction

Amphiodia occidentalis has separate sexes and are broadcast spawners,[10] releasing their eggs and sperm into the water column where fertilization and larval development occurs as plankton [11] Their breeding cycles are periodic with higher rates of spawning activity in the winter and spring.[10]

Life stages

Fertilized eggs of Amphiodia occidentalis are spherical, negatively buoyant, and surrounded by a thick hyaline layer and a fertilization envelope.[7] The larvae exhibit bilateral symmetry but lack other characteristic structures of ophiopluteus larva (such as cilia, larval arms, paired larval spicules) setting them apart from other brittle stars.[7] When they hatch out of the fertilization envelope as juveniles, they exhibit pentamerous radial symmetry. They also remain immotile for five days as they lack cilia and developed podia.[7] At day eight after fertilization, they can use their podia for movement.[7] They continue to grow and develop until they reach the adult stage.

References

  1. ↑ Stöhr, Sabine (2012). Stöhr S, O'Hara T (eds.). "Amphiodia occidentalis (Lyman, 1860)". World Ophiuroidea database. World Register of Marine Species. Retrieved 2012-10-16.
  2. ↑ "Amphiodia occidentalis, long-armed brittle star". Search SeaLifeBase. Retrieved 2021-02-11.
  3. 1 2 Fager, Edward W. (1968). "A Sand-Bottom Epifaunal Community of Invertebrates in Shallow Water". Limnology and Oceanography. 13 (3): 448–464. doi:10.4319/lo.1968.13.3.0448. ISSN 0024-3590. JSTOR 2833737.
  4. ↑ "Robert H. Morris, Donald P. Abbott & Eugene C. Haderlie, 1980. Intertidal Invertebrates of California: xi + 690 pp., 6 maps, 200 coloured plates. Stanford University Press, Stanford, California, U.S.A. ISBN 0-8047-1045-7. Price $U.S. 30.00". Crustaceana. 41 (3): 319. 1981. doi:10.1163/156854081x00930. ISSN 0011-216X.
  5. 1 2 Burgess, Dany (March 18, 2018). "The brittle stars embody nature's fragility...and resilience". Washington State Department of Ecology.
  6. ↑ Lyman, T (1860). "Descriptions of new Ophiuridae, belonging to the Smithsonian Institution and to the Museum of Comparative Zoölogy at Cambridge". Proceedings of the Boston Society of Natural History. 7: 193–204. doi:10.5962/bhl.part.4822. ISSN 0270-2444.
  7. 1 2 3 4 5 6 7 8 Emlet, Richard B. (2006-06-01). "Direct development of the brittle star Amphiodia occidentalis (Ophiuroidea, Amphiuridae) from the northeastern Pacific Ocean". Invertebrate Biology. 125 (2): 154–171. doi:10.1111/j.1744-7410.2006.00049.x.
  8. ↑ Zueva, Olga; Khoury, Maleana; Heinzeller, Thomas; Mashanova, Daria; Mashanov, Vladimir (2018). "The complex simplicity of the brittle star nervous system". Frontiers in Zoology. 15 (1): 1. doi:10.1186/s12983-017-0247-4. ISSN 1742-9994. PMC 5796562. PMID 29434647.
  9. 1 2 3 4 Astley, Henry C. (2012-06-01). "Getting around when you're round: quantitative analysis of the locomotion of the blunt-spined brittle star, Ophiocoma echinata". Journal of Experimental Biology. 215 (11): 1923–1929. doi:10.1242/jeb.068460. ISSN 1477-9145. PMID 22573771. S2CID 11314014.
  10. 1 2 Rumrill, Steven S.; Pearse, John S. (1985), "Contrasting reproductive periodicities among north-eastern Pacific ophiuroids", Echinodermata, CRC Press, doi:10.1201/9781003079224-137, ISBN 978-1-003-07922-4, S2CID 225438754, retrieved 2022-04-24
  11. ↑ Stöhr, Sabine; O'Hara, Timothy D.; Thuy, Ben (2012-03-02). Laudet, Vincent (ed.). "Global Diversity of Brittle Stars (Echinodermata: Ophiuroidea)". PLOS ONE. 7 (3): e31940. doi:10.1371/journal.pone.0031940. ISSN 1932-6203. PMC 3292557. PMID 22396744.
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