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Flood Basalts and Mass Extinctions |
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There is a strong correlation between continental flood basalts and mass extinctions (Courtillot, 1994). The three largest known mass extinctions coincide with the three largest Phanerozoic flood basalt provinces (P-Tr - Siberian Traps; Tr-J - CAMP; K-T - Deccan), within error of the sampling and dating methods. Furthermore, there are strong correlations between flood basalts and other indicators of system stress. For example, the Karoo-Ferrar Province correlates with a major oceanic anoxic event 189 m.y. ago, and part of the North Atlantic Igneous Province coincides with the Late Palaeocene Thermal Maximum, 55 m.y. ago. Despite searches, no comparable correlation exists between meteorite or cometary impacts and mass extinctions. These 'matches' are too fortuitous to be pure chance (White and Saunders, 2005), but an understanding of the actual causal link between a flood basalt event and a mass extinction is elusive. It is also worth mentioning that some flood basalts (e.g. the Parana) do not match with any indicators of serious system stress, and some small mass extinctions do not appear to correspond with any flood basalts. This may be because it is unlikely that there is one single cause for all mass extinctions. |
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Figure Caption: Extinction rate versus time (continuous line, blue field) (multiple-interval marine genera, modified from Sepkoski, 1996) compared with eruption ages of continental flood basalts (red columns). Three of the largest mass extinctions, the Permo-triassic, Triassic-Jurassic and the Cretaceous-Tertiary, correspond with the eruptions of the Siberian Traps, the Central Atlantic Magmatic Province, and the Deccan Traps, respectively. Three oceanic plateaus, the Caribbean (CP) Kerguelen (KP), and Ontong Java (OJP) are included. Modified after White and Saunders (2005). | |||||||||||||||||||||||
A possible scenario is that a single flood basalt eruptive event - more than 1000 cubic km - would erupt a very large mass of sulfur dioxide gas and aerosol, some of which would enter the lower stratosphere. This would reduce the amount of light reaching the Earth's surface (e.g., Thordarson and Self, 1996; Self et al., 2006). |
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