Department of Natural Resource Sciences, McGill University, 21111 Lakeshore Boulevard, Sainte-Anne-de-Bellevue, QC H9X 3V9, Canada.
National Wildlife Research Centre, Environment and Climate Change Canada, Ottawa, ON, Canada.
Curr Biol. 2022 Sep 12;32(17):3800-3807.e3. doi: 10.1016/j.cub.2022.06.084. Epub 2022 Jul 22.
Density-dependent prey depletion around breeding colonies has long been considered an important factor controlling the population dynamics of colonial animals. Ashmole proposed that as seabird colony size increases, intraspecific competition leads to declines in reproductive success, as breeding adults must spend more time and energy to find prey farther from the colony. Seabird colony size often varies over several orders of magnitude within the same species and can include millions of individuals per colony. As such, colony size likely plays an important role in determining the individual behavior of its members and how the colony interacts with the surrounding environment. Using tracking data from murres (Uria spp.), the world's most densely breeding seabirds, we show that the distribution of foraging-trip distances scales to colony size during the chick-rearing stage, consistent with Ashmole's halo theory. This pattern occurred across colonies varying in size over three orders of magnitude and distributed throughout the North Atlantic region. The strong relationship between colony size and foraging range means that the foraging areas of some colonial species can be estimated from colony sizes, which is more practical to measure over a large geographic scale. Two-thirds of the North Atlantic murre population breed at the 16 largest colonies; by extrapolating the predicted foraging ranges to sites without tracking data, we show that only two of these large colonies have significant coverage as marine protected areas. Our results are an important example of how theoretical models, in this case, Ashmole's version of central-place-foraging theory, can be applied to inform conservation and management in colonial breeding species.
繁殖地周围与种群密度相关的猎物枯竭长期以来被认为是控制群居动物种群动态的一个重要因素。阿什莫尔提出,随着海鸟繁殖地规模的增大,种内竞争导致繁殖成功率下降,因为繁殖的成年个体必须花费更多的时间和精力从更远的地方寻找猎物。海鸟繁殖地的规模在同一物种内通常会有几个数量级的变化,每个繁殖地可能有上百万只个体。因此,繁殖地的规模可能在决定其成员的个体行为以及繁殖地与周围环境的相互作用方面起着重要作用。利用来自海鸠(Uria 属)的追踪数据,这是世界上繁殖密度最高的海鸟,我们发现,在育雏阶段,觅食距离的分布与繁殖地的规模呈比例关系,这与阿什莫尔的“光环理论”一致。这种模式出现在跨越三个数量级大小的繁殖地中,分布在整个北大西洋地区。繁殖地规模与觅食范围之间的紧密关系意味着,一些群居物种的觅食区可以根据繁殖地的规模来估计,这在大地理尺度上更便于测量。北大西洋海鸠种群中有三分之二在 16 个最大的繁殖地繁殖;通过将预测的觅食范围外推到没有追踪数据的地点,我们表明,在这些大型繁殖地中,只有两个有作为海洋保护区的重要覆盖范围。我们的研究结果是一个重要的例子,说明了理论模型(在这种情况下,阿什莫尔的中心觅食理论版本)如何能够应用于群居繁殖物种的保护和管理。