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Halystina globulus

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Halystina globulus
Scientific classification Edit this classification
Domain: Eukaryota
Kingdom: Animalia
Phylum: Mollusca
Class: Gastropoda
Subclass: Vetigastropoda
Family: Seguenziidae
Genus: Halystina
Species:
H. globulus
Binomial name
Halystina globulus
Poppe, Tagaro & Dekker, 2006[1][2]

Halystina globulus is a species of sea snail, a marine gastropod mollusc in the family Seguenziidae.[3] The scientific name of Halystina globulus comes from the Greek words "Halys" (meaning sea) and "Stena" (meaning chest), referring to the location of the snail's body within its shell.[4]

Description

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Halystina globulus has a small, smooth, and glossy shell that is globular or oval-shaped, with a height of up to 5 mm and a width of up to 4 mm. The shell is thin, fragile, and translucent, with a white to yellowish-brown coloration. The snail has a small, conical spire and a round aperture with a thin, sharp outer lip. The surface of the shell is smooth, with fine and closely spaced growth lines and a few spiral lines on the base. The operculum is thin and corneous, with a brown coloration. This family of snails is known for its small size, intricate shell structures, and ability to thrive in the dark, cold, and high-pressure conditions of the deep sea. Halystina globulus, like many other members of its family, is a micromollusk, meaning that it is exceptionally small—often less than a few millimeters in size. Despite its minute stature, it plays a vital role in the ecological systems of the benthic zones, which are the lowest levels of the ocean.

Taxonomy and morphology

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Halystina globulus is classified under the kingdom Animalia, phylum Mollusca, and class Gastropoda. It belongs to the superfamily Seguenzioidea and the family Seguenziidae. The genus Halystina includes several deep-sea gastropods, all of which share similar characteristics.[5] Halystina globulus is known for its small, rounded shell, which is globular in shape—hence its name. The shell is typically smooth, with tight, compact whorls spiraling from the apex down to the aperture, which is round and simple in design. The shell is generally translucent or white in color, allowing it to blend into its deep-sea environment. Due to the extreme depths at which it lives, this snail has evolved adaptations that enable it to survive in high-pressure, low-light conditions.[6]

Distribution and habitat

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Halystina globulus is found in deep waters of the Southwest Pacific Ocean, specifically around New Zealand and Australia. Halystina globulus is a benthic species that is at depths ranging from 200 to 1,100 meters, and it typically lives on muddy or sandy substrates. It is commonly found in the southeastern Pacific Ocean, including off the coast of Chile, Peru, and Ecuador. Due to its deep-water habitat, humans do not commonly encounter the species.[7] Halystina globulus is found primarily in deep-sea environments, typically at depths ranging from 200 to over 2,000 meters. These habitats include seamounts, mid-ocean ridges, and other underwater geological formations where nutrients settle to the ocean floor.[8] These deep-sea ecosystems are rich in biodiversity, but they are also some of the least explored and understood by scientists due to the challenges of studying life at such extreme depths.[9] The snail’s small size allows it to inhabit crevices and cracks in rocky substrates or sediment layers on the ocean floor. The benthic zone, where H. globulus is typically found, is a stable yet nutrient-poor environment, and species living here have adapted to slow growth rates and low metabolic needs.

Feeding and ecology

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As a member of the deep-sea community, Halystina globulus likely feeds on detritus, microorganisms, or biofilm that accumulates on the ocean floor.[10][page needed] Deep-sea detritivores like H. globulus play a crucial role in recycling nutrients and maintaining the health of benthic ecosystems. The deep-sea food web is less diverse compared to shallower ecosystems,[11][page needed] and much of the organic matter comes from the decay of marine organisms or marine snow, a steady drift of organic particles from the upper layers of the ocean.[12] The low-light conditions of the deep sea limit photosynthesis, so species like Halystina globulus rely on scavenging detritus for sustenance. Its small size and slow metabolism allow it to survive in this low-energy environment.

Reproduction and development

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Reproductive strategies in deep-sea gastropods like Halystina globulus are not as well studied as those in shallower marine species, but it is presumed that this species reproduces through external fertilization. Many deep-sea gastropods lay eggs that develop into free-swimming larvae. These larvae may be planktonic, drifting in ocean currents before eventually settling on the ocean floor, where they undergo metamorphosis into their adult forms. The ability to disperse as larvae is crucial for species in deep-sea environments, as suitable habitats can be patchy and far between.[13] The extreme pressures and low temperatures in the deep sea may also contribute to slower growth rates and longer developmental periods compared to species in shallower waters.[14]

Conservation and threats

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Although specific conservation assessments for Halystina globulus are not available, deep-sea species in general are considered vulnerable to anthropogenic impacts, including deep-sea trawling, mining, and climate change. Deep-sea ecosystems are particularly susceptible to physical disturbances because of their slow recovery rates.[15] Many species that live in these ecosystems have low reproductive rates and long lifespans, making them slow to rebound from population declines. Additionally, deep-sea mining for minerals and resources such as polymetallic nodules, which are found on the ocean floor, poses a significant threat to these habitats. The destruction of the benthic environment could lead to the loss of species like H. globulus before they are even fully understood by science.

Scientific importance

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The study of species like Halystina globulus is essential for understanding the biodiversity of the deep sea, one of the most remote and least explored environments on Earth. Research on these organisms helps scientists learn about the adaptations necessary for survival in extreme environments, which can have broader implications for fields such as evolutionary biology, ecology, and even astrobiology.[16] The deep sea is often compared to other extreme environments, such as those found on other planets or moons, and the organisms that live there may provide insights into the potential for life beyond Earth. Additionally, deep-sea species contribute to the overall functioning of marine ecosystems, playing roles in nutrient cycling and carbon sequestration.

References

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  1. ^ Poppe, Tagaro & Dekker. 2006. Visaya Supplement: Supplement 2 Pages: 3–228. World Register of Marine Species, Retrieved 18 April 2010.
  2. ^ Poppe, Guido T.; Tagaro, Sheila P.; Dekker, Henk (2006). "The Seguenziidae, Chilodontidae, Trochidae, Calliostomatidae and Solariellidae of the Philippine Islands with the description of 1 new genus, 2 new subgenera, 70 new species and 1 new subspecies". Visaya Supplement. 2: 1–228. Retrieved 16 February 2019.
  3. ^ Halystina globulus Poppe, Tagaro & Dekker, 2006. Retrieved through: World Register of Marine Species on 18 April 2010.
  4. ^ Tipsfu (29 April 2023). "Halystina Globulus: A Fascinating Marine Gastropod Mollusk". TipsFu. Retrieved 30 April 2023.
  5. ^ Chamberlain, Scott; Vanhoorne., Bart (14 January 2017). "worrms: World Register of Marine Species (WoRMS) Client". CRAN: Contributed Packages. doi:10.32614/cran.package.worrms. Retrieved 24 October 2024.
  6. ^ Bouchet, Philippe; Rocroi, Jean-Pierre; Hausdorf, Bernhard; Kaim, Andrzej; Kano, Yasunori; Nützel, Alexander; Parkhaev, Pavel; Schrödl, Michael; Strong, Ellen E. (December 2017). "Revised Classification, Nomenclator and Typification of Gastropod and Monoplacophoran Families". Malacologia. 61 (1–2): 1–526. doi:10.4002/040.061.0201. ISSN 0076-2997.
  7. ^ Kano, Yasunori (7 December 2007). "Vetigastropod phylogeny and a new concept of Seguenzioidea: independent evolution of copulatory organs in the deep-sea habitats". Zoologica Scripta. 37 (1): 1–21. doi:10.1111/j.1463-6409.2007.00316.x. ISSN 0300-3256.
  8. ^ Watling, Les; Norse, Elliott A. (December 1998). "Disturbance of the Seabed by Mobile Fishing Gear: A Comparison to Forest Clearcutting". Conservation Biology. 12 (6): 1180–1197. Bibcode:1998ConBi..12.1180W. doi:10.1046/j.1523-1739.1998.0120061180.x. ISSN 0888-8892.
  9. ^ Levin, Lisa A.; Sibuet, Myriam (15 January 2012). "Understanding Continental Margin Biodiversity: A New Imperative". Annual Review of Marine Science. 4 (1): 79–112. Bibcode:2012ARMS....4...79L. doi:10.1146/annurev-marine-120709-142714. ISSN 1941-1405. PMID 22457970.
  10. ^ Gage, John D.; Tyler, Paul A. (18 April 1991). Deep-Sea Biology. Cambridge University Press. doi:10.1017/cbo9781139163637. ISBN 978-0-521-33431-0.
  11. ^ Van Dover, Cindy Lee (31 December 2000). The Ecology of Deep-Sea Hydrothermal Vents. Princeton University Press. doi:10.1515/9780691239477. ISBN 978-0-691-23947-7.
  12. ^ "Abundance and size structure of the deep-sea benthos", Deep-Sea Biology, Cambridge University Press, pp. 181–200, 18 April 1991, doi:10.1017/cbo9781139163637.012, ISBN 978-0-521-33431-0, retrieved 24 October 2024
  13. ^ Miller, K; Neil, H; Tracey, D (17 December 2009). "INTRODUCTION Recent advances in deep-sea coral science and emerging links to conservation and management of deep-sea ecosystems Karen Miller1,*, Helen Neil2, Di Tracey2". Marine Ecology Progress Series. 397: 1–5. Bibcode:2009MEPS..397....1M. doi:10.3354/meps08452. ISSN 0171-8630.
  14. ^ Koslow, JA; Gowlett-Holmes, K; Lowry, JK; O'Hara, T; Poore, GCB; Williams, A (2001). "Seamount benthic macrofauna off southern Tasmania: community structure and impacts of trawling". Marine Ecology Progress Series. 213: 111–125. Bibcode:2001MEPS..213..111K. doi:10.3354/meps213111. ISSN 0171-8630.
  15. ^ Ramirez-Llodra, Eva; Tyler, Paul A.; Baker, Maria C.; Bergstad, Odd Aksel; Clark, Malcolm R.; Escobar, Elva; Levin, Lisa A.; Menot, Lenaick; Rowden, Ashley A.; Smith, Craig R.; Van Dover, Cindy L. (1 August 2011). "Man and the Last Great Wilderness: Human Impact on the Deep Sea". PLOS ONE. 6 (8): e22588. Bibcode:2011PLoSO...622588R. doi:10.1371/journal.pone.0022588. ISSN 1932-6203. PMC 3148232. PMID 21829635.
  16. ^ Vinogradova, N.G. (1997), "Zoogeography of the Abyssal and Hadal Zones", The Biogeography of the Oceans, Advances in Marine Biology, vol. 32, Elsevier, pp. 325–387, doi:10.1016/s0065-2881(08)60019-x, ISBN 978-0-12-026132-1, retrieved 24 October 2024
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