Orbital forcing of deep-sea benthic species diversity
Orbital forcing of deep-sea benthic species diversity
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DOI：
10.1038/385624a0
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发表时间：
1997-02-13
期刊：
影响因子：
64.8
通讯作者：
Raymo, ME
中科院分区：
文献类型：
--
作者：
Cronin, TM;Raymo, ME
Explanations for the temporal and spatial patterns of species biodiversity focus on stability-time(1-3), disturbance-mosaic (biogenic microhabitat heterogeneity)(4,5) and competition-predation (biotic interactions)(6,7) hypotheses. The stability-time hypothesis holds that high species diversity in the deep sea and in the tropics reflects long-term climatic stability(3). But the influence of climate change on deep-sea diversity has not been studied and recent evidence suggests that deep-sea environments undergo changes in climatically driven temperature(8) and flux of nutrients(9) and organic-carbon(10) during glacial-interglacial cycles. Here we show that Pliocene (2.85-2.40 Myr) deep-sea North Atlantic benthic ostracod (Crustacea) species diversity is related to solar insolation changes caused by 41,000-yr cycles of Earth's obliquity (tilt). Temporal changes in diversity, as measured by the Shannon-Weiner index, H(S), correlate with independent climate indicators of benthic foraminiferal oxygen-isotope ratios (mainly ice volume(11-13)) and ostracod Mg:Ca ratios (bottom-water temperature(8)). During glacial periods, H(S) = 0.2-0.6, whereas during interglacials, H(S) = 1.2-1.6, which is three to four times as high. The control of deep-sea benthic diversity by cyclic climate change at timescales of 10(3)-10(4) yr does not support the stability-time hypothesis because it shows that the deep sea is a temporally dynamic environment. Diversity oscillations reflect large-scale response of the benthic community to climatically driven changes in either thermohaline circulation, bottom temperature (or temperature-related factors) and food, and a coupling of benthic diversity to surface productivity.
