Could the Late Permian deep ocean have been anoxic

نویسندگان

  • R. Zhang
  • M. J. Follows
  • J. E Grotzinger
چکیده

Models ofocean circulation and biogeochemical cy les are used to speculate bout possible m chanisms of deep-sea anoxia across the Pertoo-Triassic boundary. Two modes of likely Late Permian ocean thermohaline circulation are identified: a vigorous "therm',d mode" driven by cooling in southern polar latitudes and aweaker "haline mode" driven by evaporation fromthe subtropics. We find that the thermal mode, typical of climates such as our own, is unlikely to surpport deep-sea anoxia. The haline mode, which might exist in warm climates with enhanced hy rological cycles, can lead to significant but periodic epletion of oxygen in the Panthalassic deep o ean. However, owing tothe inherent instability of the haline mode, a deep-sea •oxia persisting for millions of ye,•u s is not clearly supported by this tudy, though mechanisms emerge which might be consistent with the observed record. The nhanced hy rological cycle (or educed oceanic d apycnal mixing) required toobtain the haline mode r main unconstrah•:d for the Late Permian.

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تاریخ انتشار 2007