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体型和底物类型调节西太平洋长棘海星(Acanthaster solaris)的运动。

Body size and substrate type modulate movement by the western Pacific crown-of-thorns starfish, Acanthaster solaris.

作者信息

Pratchett Morgan S, Cowan Zara-Louise, Nadler Lauren E, Caballes Ciemon F, Hoey Andrew S, Messmer Vanessa, Fletcher Cameron S, Westcott David A, Ling Scott D

机构信息

ARC Centre of Excellence for Coral Reef Studies, James Cook University, Townsville, Australia.

Scripps Institution of Oceanography, University of California San Diego, La Jolla, CA, United States of America.

出版信息

PLoS One. 2017 Sep 6;12(9):e0180805. doi: 10.1371/journal.pone.0180805. eCollection 2017.

DOI:10.1371/journal.pone.0180805
PMID:28877193
原文链接:https://pmc.ncbi.nlm.nih.gov/articles/PMC5587101/
Abstract

The movement capacity of the crown-of-thorns starfishes (Acanthaster spp.) is a primary determinant of both their distribution and impact on coral assemblages. We quantified individual movement rates for the Pacific crown-of-thorns starfish (Acanthaster solaris) ranging in size from 75-480 mm total diameter, across three different substrates (sand, flat consolidated pavement, and coral rubble) on the northern Great Barrier Reef. The mean (±SE) rate of movement for smaller (<150 mm total diameter) A. solaris was 23.99 ± 1.02 cm/ min and 33.41 ± 1.49 cm/ min for individuals >350 mm total diameter. Mean (±SE) rates of movement varied with substrate type, being much higher on sand (36.53 ± 1.31 cm/ min) compared to consolidated pavement (28.04 ± 1.15 cm/ min) and slowest across coral rubble (17.25 ± 0.63 cm/ min). If average rates of movement measured here can be sustained, in combination with strong directionality, displacement distances of adult A. solaris could range from 250-520 m/ day, depending on the prevailing substrate. Sustained movement of A. solaris is, however, likely to be highly constrained by habitat heterogeneity, energetic constraints, resource availability, and diurnal patterns of activity, thereby limiting their capacity to move between reefs or habitats.

摘要

棘冠海星(刺冠海星属)的移动能力是决定其分布范围以及对珊瑚群落影响程度的主要因素。我们对总直径在75 - 480毫米之间的太平洋棘冠海星(Acanthaster solaris)个体移动速率进行了量化,研究范围涵盖了大堡礁北部三种不同的基质(沙地、平坦的固结路面和珊瑚 rubble)。总直径小于150毫米的小型A. solaris平均(±标准误)移动速率为23.99 ± 1.02厘米/分钟,而总直径大于350毫米的个体平均移动速率为33.41 ± 1.49厘米/分钟。平均(±标准误)移动速率因基质类型而异,在沙地(36.53 ± 1.31厘米/分钟)上的移动速率远高于固结路面(28.04 ± 1.15厘米/分钟),在珊瑚 rubble上移动最慢(17.25 ± 0.63厘米/分钟)。如果此处测得的平均移动速率能够持续,再结合较强的方向性,成年A. solaris的每日位移距离可能在250 - 520米之间,具体取决于主要的基质类型。然而,A. solaris的持续移动很可能会受到栖息地异质性、能量限制、资源可用性以及昼夜活动模式的高度制约,从而限制它们在珊瑚礁或栖息地之间移动的能力。

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