OFR 151.pdf - CRC LEME
OFR 151.pdf - CRC LEME
OFR 151.pdf - CRC LEME
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7.1. Global backdrop<br />
SECTION 7 (TERTIARY CLIMATES)<br />
During the Tertiary, the earth as a whole underwent progressive warming, then cooling/drying<br />
episodes (Frakes 1999). Although no single factor is likely to be paramount in any region,<br />
patterns of Tertiary climatic change are increasingly being linked to changes in deep ocean<br />
circulation associated with continental drift (Zachos et al. 1994).<br />
As in the Cretaceous, global trends were interrupted or sharpened by a number of short-term<br />
climatic excursions whose impact was variable. For example, there is increasing evidence<br />
that the earth suffered a number of major impacts from extraterrestrial bolides during the<br />
Tertiary although the climatic consequences continue to be debated. Farley et al. (1998) cite<br />
geochemical evidence for a comet shower extending over a 2.5 million year period in the Late<br />
Eocene. Two impacts produced major craters – off the East Coast of America (Chesapeake<br />
Bay Crater) and in Siberia (Popigai Crater). The more important of these geologically shortterm<br />
climatic excursions are: the Cretaceous-Tertiary boundary event at about 65 Ma; the<br />
Paleocene-Eocene Thermal Maximum at about 55 Ma; and four events linked to changes in<br />
ocean circulation, being the Eocene-Oligocene transition linked to the opening of the<br />
Tasmanian Gateway between Australia and Antarctica at about 33 Ma, the mid Miocene<br />
climatic transition between 21-27 Ma, mid Pliocene warming at about 3 Ma and Plio-<br />
Pleistocene bipolar glaciation after 2.5 Ma.<br />
7.1.1 Cretaceous-Tertiary boundary (K/T) event [~65 Ma]<br />
A number of events, which began during the late Late Cretaceous, culminated near to, but<br />
before, the Cretaceous-Tertiary (K/T) boundary. These range from abnormally high levels of<br />
volcanism (Sutherland 1994) and increased terrestrial erosion (Robert and Chamley 1990) to a<br />
decline in dinosaur diversity (Sereno 1999) and major changes in climate and ocean chemistry<br />
(Barrera 1994).<br />
A common explanation is marine regression during the latest Maastrichtian, e.g. Barrera et al.<br />
(1997) and Eaton et al. (1997). Nevertheless, unlike earlier geological boundaries, the<br />
evidence is compelling that the Cenozoic era was initiated by the impact of a ~10 km<br />
diameter bolide moving at ~20 km sec -1 at Chicxulub in the Gulf of Mexico (Hildebrand et al.<br />
1995, Melosh 1995, Kerr 1997, Kroon et al. 1998). Shocked quartz has been recorded as far<br />
north as the Gosau Basin in Austria (Preisinger et al. 1986). More immediate effects include<br />
the deposition of impact breccias up to 900 m thick at a distance of 100 km from the crater,<br />
the collapse of the shelf margin and emplacement of tsunami (megawave) deposits on the<br />
continental shelves in Texas and northern Mexico (references in Keller et al. 1997, Bralower<br />
et al. 1998).<br />
Observed or predicted global-scale phenomena include abrupt mortality in pelagic organisms<br />
(Paul and Mitchell 1994, Kaiho et al. 1999), collapse of deepwater benthic foraminiferal<br />
communities (Coccioni and Galeotti 1994), massive reduction in marine productivity (Barrera<br />
and Keller 1994), a world-encompassing dust cloud (Covey et al. 1994), cooling due to<br />
sulphur released into the atmosphere (Ward 1995), acid-rain (D’Hondt et al. 1994), the<br />
possible collapse of the hydrological cycle (cf. Covey et al. 1994, Vonhof and Smit 1997), the<br />
geologically instantaneous combustion of ~18-24% of the terrestrial above-ground biomass<br />
(Ivany and Salawitch 1993, Arinobu et al. 1999), lava outpouring in India (Geotimes 1995),<br />
and the release and ignition of huge amounts of methane trapped in seafloor sediments (Day<br />
1999).<br />
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