Astropecten polyacanthus
Astropecten polyacanthus | |
---|---|
Scientific classification | |
Kingdom: | Animalia |
Phylum: | Echinodermata |
Subphylum: | Eleutherozoa |
Class: | Asteroidea |
Order: | Paxillosida |
Family: | Astropectinidae |
Genus: | Astropecten |
Species: | A. polyacanthus |
Binomial name | |
Astropecten polyacanthus Müller and Troschel, 1842 [1] | |
Synonyms[1] | |
|
Astropecten polyacanthus, the sand sifting starfish or comb star, is a sea star of the family Astropectinidae. It is the most widespread species in the Astropecten genus, found throughout the Indo-Pacific region. The armspread is up to 20 cm (8 in).[2] The specific epithet "polyacanthus" comes from the Latin meaning "many thorned".[3]
Description
The upper surface of the comb star is a dark purplish colour, while the underside is orange. On the upper surface paxillae, (Latin, "little stakes") little pillars with flattened summits, are cream, grey or brown, the colours sometimes making a chevron pattern. Along the edges of the five arms there is a fringe of long, sharp marginal spines, usually with brown bases and pale tips. The arms are fairly broad and have a maximum length of 9 centimetres (3.5 in).[1] The tube feet are pointed rather than having suckers, an arrangement that is more suitable for digging.[3] Astropecten polyacanthus can be confused with Archaster spp. which look similar because both have developed features to enable them to dig through sand through convergent evolution. Archaster has spines that are flat and blunt and on its upper surface has parallel, radial rows of plates while Astropecten polyacanthus does not.[4]
Distribution
The comb star is found in shallow tropical and sub-tropical seas throughout the Indo-Pacific region from the Red Sea and Zanzibar to Hawaii, and from Japan to Australia and New Zealand. In Australia the range extends from Cape Naturaliste in the west, round the north coast to Sydney in the east. It is often found on silty sand bottoms in harbours and estuaries.[5] It is found at depths down to about 185 metres (607 ft).[1]
Biology
The comb star spends much of its time buried in the silty seabed. It feeds on detritus and bivalve and gastropod molluscs which it swallows whole. It also sometimes engulfs pebbles and digests the biofilm and small invertebrates adhering to the surface.[3]
Astropecten polyacanthus contains the potent neurotoxin, tetrodotoxin, also known as TTX which has no known antidote.[6] In a case of paralytic poisoning in Japan it was found that the victim had eaten a trumpet shell, Charonia lampas, which had acquired the toxin through its food chain, thus implicating Astropecten polyacanthus. In a study that followed this incident, most of the 54 comb stars assayed contained TTX, with one individual having a toxicity score of 520 mouse units per gram.[6]
Use in aquaria
The comb star is sometimes kept in reef aquaria where it is efficient at clearing detritus and uneaten food from the sand or gravel. It is mostly nocturnal and needs to be acclimatized gradually to the conditions in the tank. If it is overstocked, it will starve.[7]
References
- ↑ 1.0 1.1 1.2 1.3 Mah, Christopher (2012). C. L. Mah, ed. "Astropecten polyacanthus Müller & Troschel, 1842". World Asteroidea database. World Register of Marine Species. Retrieved 2012-04-07.
- ↑ Miller, M.; Batt, G. (1973). Reef and Beach Life of New Zealand. Auckland, New Zealand: William Collins (New Zealand) Ltd.
- ↑ 3.0 3.1 3.2 Astropecten polyacanthus - Comb seastar JulianRocks.net. Retrieved 2012-04-07.
- ↑ Telling Apart Sand Stars: Archaster vs. Astropecten! Two Common Trade Species Echinoblog. Retrieved 2012-04-07.
- ↑ Comb Seastar (Astropecten polyacanthus) Scuba Equipment USA. Retrieved 2012-04-07.
- ↑ 6.0 6.1 Miyazawa, K.; Noguchi,T.; Maruyama, J.; Jeon, J. K.; Otsuka, M.; Hashimoto, K. (1985). "Occurrence of tetrodotoxin in the starfishes Astropecten polyacanthus and A. scoparius in the Seto Inland Sea". Marine Biology 90 (1): 61–64. doi:10.1007/BF00428215.
- ↑ Astropecten polyacanthus - Sand Sifting Starfish Blue Zoo Aquatics. Retrieved 2012-04-07.