Threshold dynamics of mass extinctions and human famine risk

Evolving Earth Pub Date : 2026-01-01 Epub Date: 2026-02-18 DOI:10.1016/j.eve.2026.100114
Kunio Kaiho
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Abstract

Large-scale continental volcanism, meteoroid impacts, and nuclear war can inject massive amounts of sulfur dioxide or soot into the stratosphere, causing solar dimming, global cooling, reduced rainfall, and—at extremes—global famine and mass extinction. Using Phanerozoic data, this study quantifies animal extinction magnitudes and human famine risk under such scenarios. We find a nonlinear threshold: species loss surges from a few percent to 20–40% when soot exceeds 100–120 Tg or volcanic ejecta surpasses 500,000–700,000 km3. Human population loss from food shortages increases more gradually, reaching 50–80% beyond these thresholds. These tipping points may be exceeded by massive eruptions, large asteroid impacts, or full-scale nuclear war. Our results offer a unified model for extinction mechanisms and underscore the grave risks these events pose to biodiversity and human survival.

Abstract Image

大规模物种灭绝和人类饥荒风险的阈值动态
大规模的大陆火山活动、流星体撞击和核战争会将大量的二氧化硫或烟尘注入平流层,导致太阳变暗、全球变冷、降雨量减少,在极端情况下,还会导致全球饥荒和大规模物种灭绝。利用显生宙的数据,本研究量化了这种情景下动物灭绝的程度和人类饥荒的风险。我们发现了一个非线性阈值:当烟尘超过100-120 Tg或火山喷出物超过50 - 700,000 km3时,物种损失从几个百分点激增到20-40%。粮食短缺造成的人口损失增加更为缓慢,超过这些阈值的50% - 80%。这些临界点可能会被大规模火山喷发、大型小行星撞击或全面核战争所超越。我们的研究结果为灭绝机制提供了一个统一的模型,并强调了这些事件对生物多样性和人类生存构成的严重风险。
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