Giant mobile coralliths from the Florida Keys, USA

IF 1.5 4区 地球科学 Q3 MARINE & FRESHWATER BIOLOGY Bulletin of Marine Science Pub Date : 2023-01-01 DOI:10.5343/bms.2023.0051
William F Precht, Mark R Patterson, Peter W Glynn
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Abstract

Coralliths are spherical, free-living (motile), scleractinian colonies inhabiting present day and ancient coral reefs. They form by the coral rolling on the seabed which can occur through biological and/or physical processes. While diving and snorkeling in nearshore environments in the upper Florida Keys, we observed hundreds of coralliths of varying sizes and species. This included colonies of Porites astreoides, Siderastrea radians, and Solenastrea bournoni . The largest coralliths we observed were all S. bournoni and ranged between 0.5 and 1.4 m in diameter. The exceptionally large colonies identified (>1 m) may be the largest and oldest spherical coralliths described to date. Relatively frequent movement of a corallith is key to their formation as all colony surfaces must be exposed to sunlight and currents periodically to maintain their spherical shape. Intuitively, the larger a corallith grows, the stronger the current energy must be to initiate movement. Considering the shallow depth of the corallith habitat and the high frequency of tropical storms and hurricanes impacting south Florida, we hypothesized that the forces generated by shoaling, breaking storm waves would be sufficient to cause the formation of these giant coralliths. Calculations based on hydrodynamic forces and field observations after the passage of a storm support the efficacy of storm-generated waves and surge to move and roll these giant coralliths. The tropical storm/hurricane return time where we found these large colonies in the Florida Keys is one in every seven years. This return time is apparently frequent enough to maintain their spherical morphology and assist in the formation of these giant coralliths.
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来自美国佛罗里达群岛的巨型移动珊瑚
珊瑚虫是球形的、自由生活的(可移动的)、硬核动物群落,生活在现在和古代的珊瑚礁中。它们是由珊瑚在海床上滚动形成的,这可以通过生物和/或物理过程发生。在佛罗里达群岛上的近岸环境中潜水和浮潜时,我们观察到了数百种不同大小和种类的珊瑚。这包括了小行星、弧度星和波诺尼星的殖民地。我们观察到的最大珊瑚都是S. bournoni,直径在0.5 ~ 1.4 m之间。发现的特别大的珊瑚群(1米)可能是迄今为止描述的最大和最古老的球形珊瑚。珊瑚体相对频繁的运动是它们形成的关键,因为所有的珊瑚群表面必须周期性地暴露在阳光和水流中,以保持它们的球形。直观地说,珊瑚体越大,启动运动的电流能量就必须越强。考虑到珊瑚栖息地的深度较浅,热带风暴和飓风对南佛罗里达的影响频率很高,我们假设,浅滩和风暴波浪产生的力量足以导致这些巨大珊瑚的形成。基于水动力的计算和风暴通过后的现场观测支持了风暴产生的波浪和浪涌移动和滚动这些巨大珊瑚的功效。我们在佛罗里达群岛发现这些大型群落的热带风暴/飓风回归时间是每七年一次。这种返回时间显然足够频繁,足以维持它们的球形形态,并有助于这些巨大珊瑚的形成。
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来源期刊
Bulletin of Marine Science
Bulletin of Marine Science 地学-海洋学
CiteScore
2.90
自引率
6.70%
发文量
25
审稿时长
6-12 weeks
期刊介绍: The Bulletin of Marine Science is a hybrid open access journal dedicated to the dissemination of research dealing with the waters of the world’s oceans. All aspects of marine science are treated by the Bulletin of Marine Science, including papers in marine biology, biological oceanography, fisheries, marine policy, applied marine physics, marine geology and geophysics, marine and atmospheric chemistry, meteorology, and physical oceanography. In most regular issues the Bulletin features separate sections on new taxa, coral reefs, and novel research gear, instrument, device, or system with potential to advance marine research (“Research Tools in Marine Science”). Additionally, the Bulletin publishes informative stand-alone artwork with accompany text in its section "Portraits of Marine Science."
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