DiscoverSpeciesOther invertebrates
Haplosyllis spongicola
- Usual depth2–340 m
- Water temperature9–30 °C
- Best monthsJune and August
- How commonOccasional
About this species
Haplosyllis spongicola, the sponge worm, is a species of polychaete worm in the family Syllidae. It was previously classified as Syllis spongicola and is part of a species complex of closely related species that are difficult to distinguish morphologically and where the demarcation between them is unclear. It is found in shallow temperate, subtropical and tropical seas worldwide, wherever its host sponges are found.
Text from the Wikipedia article “Haplosyllis spongicola”, licensed CC BY-SA 4.0. Read the article
Where and when
Where it has been recorded
Worldwide
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Best months
Worldwide (open data)
- January: 89 records
- February: 56 records
- March: 26 records
- April: 61 records
- May: 67 records
- June: 165 records
- July: 133 records
- August: 242 records
- September: 138 records
- October: 57 records
- November: 39 records
- December: 28 records
Depth and water temperature
Depth
Mostly recorded at 2–340 m · Deepest record: 1,175 m
Water temperature
Recorded in surface water of 9–30 °C
Names and classification
Names in 1 more languages
- Japanese
- カイメンシリス
Other scientific names: Eusyllis setubalensis, Haplosyllis (Syllis) hamata, Haplosyllis hamata, Haplosyllis maderensis, Haplosyllis oligochaeta, Haplosyllis palpata, Hemisyllis dispar, Nereis teticola, Syllis (Haplosyllis) hamata, Syllis (Haplosyllis) spongicola, Syllis hamata, Syllis oligochaeta, Syllis setubalensis, Syllis spongicola
Similar species
Sources and credits
Names and taxonomy: WoRMS (CC BY 4.0) and the GBIF Backbone (CC BY 4.0). Photos: iNaturalist observers, each under the licence shown (CC0, CC BY or CC BY-SA).
- Depth, temperature, months and maps: records from OBIS and GBIF under CC0 or CC BY.
- Descriptions: Wikipedia, licensed CC BY-SA, each linked to its article.
- Conservation status as published by GBIF (IUCN Red List).
- 1,485 open-data records from 1855 to 2023.
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