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Spatio–temporal variation in stable isotope signatures (δ13C and δ15N) of sponges on the Saba Bank

机译:萨巴河岸海绵的稳定同位素特征(δ13C和δ15N)的时空变化

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摘要

Sponges are ubiquitous on coral reefs, mostly long lived and therefore adaptive to changing environmental conditions. They feed on organic matter withdrawn from the passing water and they may harbor microorganisms (endosymbionts), which contribute to their nutrition. Their diets and stable isotope (SI) fractionation determine the SI signature of the sponge holobiont. Little is known of spatio–temporal variations in SI signatures of δ13C and δ15N in tropical sponges and whether they reflect variations in the environment. We investigated the SI signatures of seven common sponge species with different functional traits and their potential food sources between 15 and 32 m depth along the S-SE and E-NE side of the Saba Bank, Eastern Caribbean, in October 2011 and October 2013. SI signatures differed significantly between most sponge species, both in mean values and in variation, indicating different food preferences and/or fractionation, inferring sponge species-specific isotopic niche spaces. In 2011, all sponge species at the S-SE side were enriched in d13C compared to the E-NE side. In 2013, SI signatures of sponges did not differ between the two sides and were overall lighter in δ13C and δ15N than in 2011. Observed spatio–temporal changes in SI in sponges could not be attributed to changes in the SI signatures of their potential food sources, which remained stable with different SI signatures of pelagic (particulate organic matter (POM): δ13C −24.9‰, δ15N +4.3‰) and benthic-derived food (macroalgae: δ13C −15.4‰, δ15N +0.8‰). Enriched δ13C signatures in sponges at the S-SE side in 2011 are proposed to be attributed to predominantly feeding on benthic-derived C. This interpretation was supported by significant differences in water mass constituents between sides in October 2011. Elevated NO3 and dissolved organic matter concentrations point toward a stronger reef signal in reef overlying water at the S-SE than N-NE side of the Bank in 2011. The depletions of δ13C and δ15N in sponges in October 2013 compared to October 2011 concurred with significantly elevated POM concentrations. The contemporaneous decrease in δ15N suggests that sponges obtain their N mostly from benthic-derived food with a lower δ15N than pelagic food. Average proportional feeding on available sources varied between sponge species and ranged from 20% to 50% for benthic and 50% to 80% for pelagic-derived food, assuming trophic enrichment factors of 0.5‰ ± sd 0.5 for δ13C and 3‰ ± sd 0.5 for δ15N for sponges. We suggest that observed variation of SI in sponges between sides and years were the result of shifts in the proportion of ingested benthic- and pelagic-derived organic matter driven by environmental changes. We show that sponge SI signatures reflect environmental variability in space and time on the Saba Bank and that SI of sponges irrespective of their species-specific traits move in a similar direction in response to these environmental changes.
机译:海绵在珊瑚礁上无处不在,大多寿命长,因此可以适应不断变化的环境条件。它们以从流水中抽出的有机物为食,并且可能藏有有助于其营养的微生物(内共生菌)。它们的饮食和稳定的同位素(SI)分级确定了海绵状全卤虫的SI特征。关于热带海绵中δ 13 C和δ 15 N的SI特征的时空变化以及它们是否反映了环境变化的知之甚少。我们在2011年10月和2013年10月对东加勒比沙巴银行的S-SE和E-NE侧调查了具有不同功能性状的7种常见海绵物种的SI标记及其潜在的食物来源,深度在15至32 m之间。在大多数海绵物种之间,SI签名的平均值和变异性均存在显着差异,表明不同的食物偏爱和/或分级分离,从而推断出海绵物种特定的同位素生态位空间。 2011年,与E-NE一侧相比,S-SE一侧的所有海绵物种均富含d 13 C。 2013年,海绵的SI特征在两侧没有差异,并且δ 13 C和δ 15 N总体上比2011年轻。海绵中的SI不能归因于其潜在食物来源的SI标记的变化,这种变化在中上层(颗粒有机物(POM):δ 13 C -24.9‰, δ 15 N + 4.3‰)和底栖食物(宏藻类:δ 13 C -15.4‰,δ 15 N + 0.8‰) 。有人认为,2011年南北向海海绵中富含的δ 13 C特征归因于以底栖动物衍生的C为主要摄食。 2011年10月。2011年10月,NO-3含量升高和溶解有机物浓度增加,表明S-SE礁上覆水中的礁石信号要强于本银行N-NE一侧。δ 13 C和与2011年10月相比,2013年10月海绵中的δ 15 N表示POM浓度显着升高。 δ 15 N的同时下降表明,海绵中的N主要来自底栖食物,而δ 15 N比远洋食物低。假设δ 13的营养富集因子为0.5‰±sd 0.5,海底食物的平均比例摄食因海绵种类而异,底栖动物为20%至50%,中上层食物为50%至80%。海绵的δ 15 N的sup> C和3‰±sd 0.5。我们认为,观察到的海绵中SI的变化在侧面和侧面之间是由于环境变化驱动的底栖和浮游来源的有机物摄入比例变化的结果。我们表明,海绵SI的特征反映了萨巴河银行在空间和时间上的环境变异性,并且海绵的SI不论其特定于物种的性状如何响应这些环境变化都朝着相似的方向移动。

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