Daniel López Casares, José Carlos Hernández Pérez, José Tena Medialdea, José Rafael García March
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For each of the recorded starfish, data about the size, the substrate on which it was found, the area, the depth and the sex in the case of observing the reproduction were collected. \nResults: A total of 19 samplings have been carried out throughout a year of study. In this way, it has been possible to observe that the density of individuals increases in the shallower zone during autumn and winter, when the temperature drops to 14.13 ºC, while it decreases in spring and summer when the temperature rises to 27.17 ºC. Those results are reversed in the deepest part of the study. The highest density of individuals (0.51 ind/m2) occurred in October. Arborescent photophilic algae and crustose coralline algae were the substrates with the highest number of E. sepositus recorded. Medium to large specimens are located preferably on crustose coralline algae or arborescent photophilic algae, while smaller individuals were mostly located on Posidonia oceanica. No specimens of E. sepositus were observed spawning. \nConclusions: Data leads to assume that there is a migration of starfishes towards more superficial areas when the water is at colder temperature and towards deeper areas when the temperature increases. It is valued the possibility that there is a change in the nutritional needs of E. sepositus throughout its development. According to our observations, the future reproduction studies should be concentrated between late-summer and early-autumn.","PeriodicalId":504082,"journal":{"name":"Revista de Biología Tropical","volume":"52 10","pages":""},"PeriodicalIF":0.0000,"publicationDate":"2024-03-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Preliminary study of the population and reproductive dynamics of Echinaster sepositus (Spinulosida: Echinasteridae) in Cala del Racó\",\"authors\":\"Daniel López Casares, José Carlos Hernández Pérez, José Tena Medialdea, José Rafael García March\",\"doi\":\"10.15517/rev.biol.trop..v72is1.58967\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"Introduction: The red starfish (Echinaster sepositus) is one of the most common asteroid species in the Mediterranean Sea. However, information about their biology or their role in benthic communities is scarce. \\nObjective: This study aims to provide new information on the ecology of this species through the temporal characterization of the population of E. sepositus in Cala del Racó (Alicante, Spain) and the in situ monitoring of its reproductive cycle. \\nMethods: For this purpose, three study areas were established at different depths. For each of the recorded starfish, data about the size, the substrate on which it was found, the area, the depth and the sex in the case of observing the reproduction were collected. \\nResults: A total of 19 samplings have been carried out throughout a year of study. In this way, it has been possible to observe that the density of individuals increases in the shallower zone during autumn and winter, when the temperature drops to 14.13 ºC, while it decreases in spring and summer when the temperature rises to 27.17 ºC. Those results are reversed in the deepest part of the study. The highest density of individuals (0.51 ind/m2) occurred in October. Arborescent photophilic algae and crustose coralline algae were the substrates with the highest number of E. sepositus recorded. Medium to large specimens are located preferably on crustose coralline algae or arborescent photophilic algae, while smaller individuals were mostly located on Posidonia oceanica. No specimens of E. sepositus were observed spawning. \\nConclusions: Data leads to assume that there is a migration of starfishes towards more superficial areas when the water is at colder temperature and towards deeper areas when the temperature increases. It is valued the possibility that there is a change in the nutritional needs of E. sepositus throughout its development. 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引用次数: 0
摘要
简介红海星(Echinaster sepositus)是地中海最常见的小行星物种之一。然而,有关其生物学特性或在底栖生物群落中的作用的信息却很少。研究目的本研究旨在通过对 Cala del Racó(西班牙阿利坎特)的 E. sepositus 种群的时间特征进行描述,并对其繁殖周期进行现场监测,从而提供有关该物种生态学的新信息。研究方法:为此,在不同深度建立了三个研究区域。对记录到的每只海星,都收集了有关其大小、发现时的底质、面积、深度以及观察繁殖时的性别等数据。结果:在一年的研究中,共进行了 19 次采样。通过这种方法可以观察到,秋冬季节气温降至 14.13 ºC 时,较浅区域的个体密度会增加,而春夏季气温升至 27.17 ºC 时,个体密度会减少。这些结果在研究的最深处正好相反。10 月份个体密度最高(0.51 ind/m2)。记录到的 E. sepositus 数量最多的底质是树生嗜光藻和壳状珊瑚藻。中型到大型标本喜欢栖息在壳状珊瑚藻或乔木色嗜光藻上,而小型标本则主要栖息在海鞘上。没有观察到 E. sepositus 的产卵标本。结论数据表明,当水温较低时,星鱼会向较浅的区域迁移,而当温度升高时,则会向较深的区域迁移。值得重视的是,海星在整个发育过程中对营养的需求可能会发生变化。根据我们的观察,未来的繁殖研究应集中在夏末秋初。
Preliminary study of the population and reproductive dynamics of Echinaster sepositus (Spinulosida: Echinasteridae) in Cala del Racó
Introduction: The red starfish (Echinaster sepositus) is one of the most common asteroid species in the Mediterranean Sea. However, information about their biology or their role in benthic communities is scarce.
Objective: This study aims to provide new information on the ecology of this species through the temporal characterization of the population of E. sepositus in Cala del Racó (Alicante, Spain) and the in situ monitoring of its reproductive cycle.
Methods: For this purpose, three study areas were established at different depths. For each of the recorded starfish, data about the size, the substrate on which it was found, the area, the depth and the sex in the case of observing the reproduction were collected.
Results: A total of 19 samplings have been carried out throughout a year of study. In this way, it has been possible to observe that the density of individuals increases in the shallower zone during autumn and winter, when the temperature drops to 14.13 ºC, while it decreases in spring and summer when the temperature rises to 27.17 ºC. Those results are reversed in the deepest part of the study. The highest density of individuals (0.51 ind/m2) occurred in October. Arborescent photophilic algae and crustose coralline algae were the substrates with the highest number of E. sepositus recorded. Medium to large specimens are located preferably on crustose coralline algae or arborescent photophilic algae, while smaller individuals were mostly located on Posidonia oceanica. No specimens of E. sepositus were observed spawning.
Conclusions: Data leads to assume that there is a migration of starfishes towards more superficial areas when the water is at colder temperature and towards deeper areas when the temperature increases. It is valued the possibility that there is a change in the nutritional needs of E. sepositus throughout its development. According to our observations, the future reproduction studies should be concentrated between late-summer and early-autumn.