Sea Cucumbers and Brittle Stars Codexery

Ophiactis savignyi

A widespread brittle star that reproduces both sexually and by fragmentation.

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Ophiactis savignyi, commonly known as Savigny's brittle star or the little brittle star, is a species of brittle star in the family Ophiactidae. It is thought to be the brittle star with the most widespread distribution, occurring in tropical and subtropical parts of all the world's oceans.

Scientific classification

  1. KingdomAnimalia
  2. PhylumEchinodermata
  3. ClassOphiuroidea
  4. OrderOphiurida
  5. FamilyOphiactidae
  6. GenusOphiactis
  7. SpeciesOphiactis savignyi

Named by (Müller & Troschel, 1842)

Sources: Wikipedia taxobox: Ophiactis savignyi (CC BY-SA 4.0) · differs from this box at order: WoRMS AphiaID 125122 (CC BY 4.0)

Where the ophiactis savignyi has been recorded

Where the ophiactis savignyi has been recorded200 mapped locations from 3,682 GBIF occurrence records

Each dot is a place where the species has been observed and reported (3,682 records, half-degree grid) — not a modelled range. 77 inland records left out (institution coordinates).

Map: drawn by Codexery. Data: GBIF occurrence search (records CC0 / CC BY) · Natural Earth basemap (public domain)

Background

Ophiactis savignyi was first described in 1842 by the German zoologists Johannes Peter Müller and Franz Hermann Troschel. The specific name honors the French zoologist Marie Jules César Savigny.

The disc is up to 5 mm in diameter, with a pale greenish-brown aboral surface covered by large overlapping scales and a scattering of spines. The six arms are long, slender, and tapering, each segment bearing five or six thorny spines. The oral surface is cream-colored.

This brittle star has a near cosmopolitan distribution in warm seas, occurring in the western Indo-Pacific, eastern Pacific, and on both sides of the Atlantic. Populations in the Pacific and Atlantic were only united after the Panama Canal was cut in 1914. It is found from the intertidal zone down to about 500 meters, in reefs, mangroves, seagrass meadows, among seaweeds, and in contaminated waters, often living inside sponges possibly as a commensal.

O. savignyi is a deposit feeder and scavenger, feeding on detritus. It raises arm tips to detect food, rolls nutritious items into a ball, and moves them to the mouth using tube feet. Stomach contents have included bryozoans, foraminiferans, and gastropods among detritus and sand grains.

Individuals are either male or female and can reproduce sexually or asexually by fragmentation. In Taiwan, mature gametes occur from March to December, with peak spawning in May and June; fission occurs mostly between July and December. Sampling found 48% of individuals were regenerating, and the sex ratio was 24 males per female.

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Test yourself

Three questions drawn from this entry’s sources. Pick an answer to check it.

1. Who first scientifically described the Ophiactis savignyi?

Correct.

Not quite. The answer is Franz Hermann Troschel.

From the source: “It was first described by the German zoologists Johannes Peter Müller and Franz Hermann Troschel in 1842.”

2. In what year was Ophiactis savignyi first scientifically described?

Correct.

Not quite. The answer is 1842.

From the source: “It was first described by the German zoologists Johannes Peter Müller and Franz Hermann Troschel in 1842.”

3. To which biological family does the Ophiactis savignyi belong?

Correct.

Not quite. The answer is Ophiactidae.

From the source: “Ophiactis savignyi is a species of brittle star in the family Ophiactidae, commonly known as Savigny's brittle star or the little brittle star.”

Answers checked against the source article

Sources

Compiled from Wikipedia and the sources listed below. Text from Wikipedia is available under CC BY-SA 4.0; this entry is adapted from it.

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