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  • 1
    Electronic Resource
    Electronic Resource
    Springer
    International journal of earth sciences 46 (1959), S. 576-601 
    ISSN: 1437-3262
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences
    Notes: Abstract The Pleistocene, and possibly also other, older glaciations, are believed to have resulted from a combination of terrestrial and astronomical factors. Preceding glaciation, orogenesis and uplift increased the Earth's albedo and decreased temperature. Lowering of temperature below a certain threshold value permitted the astronomical cause to become operative. While smaller glaciations may have been largely or entirely patterned by the astronomical cause or causes, terrestrial factors had an important effect in determining the course of the larger glaciations. Two time-delay factors are believed to have been responsible for the oscillatory pattern of glaciation: these are plastic iceflow, and crustal warping. Summer insolation variation in the high latitudes is believed to be a more likely astronomical cause than variation of solar radiation.
    Type of Medium: Electronic Resource
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  • 2
    Electronic Resource
    Electronic Resource
    Springer
    International journal of earth sciences 81 (1992), S. 791-794 
    ISSN: 1437-3262
    Source: Springer Online Journal Archives 1860-2000
    Topics: Geosciences
    Notes: Abstract The giant impact on Earth proposed by some to generate the Moon could not have happened because the amount of carbonate rock and organic carbon present on Earth closely approximates the amount of CO2 predicted for the Earth's early atmosphere by comparison with the present atmosphere of Venus. It is suggested that the Moon may have fissioned from Mercury more than 4.4 billion years ago and may have been captured by the Earth no later than 3.2 billion years ago. A model for the origin of the Earth-Moon system that has been gaining favor recently visualizes a Marssize body impacting Earth and excavating enough material from the Earth to form the Moon (Newsome &Taylor, 1989). This giant impact not only would have sterilized the planet (Maher &Stevenson, 1988), obliterating any form of life that might have existed at the time, but also would have blown off the Earth's atmosphere (Kaula, 1990). As the story goes, Venus suffered no giant impact and conserved its CO2 atmosphere, whereas the loss of her CO2 atmosphere cooled the Earth's surface allowing the oceans to rain out (Kaula, 1990). It is widely believed that the different histories in the early evolution of their atmospheres set markedly different courses for the subsequent evolution of the two planets. I agree with this conclusion but disagree with the cause for the difference. If the giant impact really happened, it must have taken place not only after the Earth's accumulation was practically completed but also after a substantial core had formed (to account for the lesser density of the Moon). Venus has approximately 89 kg/cm2 of CO2 for a total of 4.11020kg. The Earth with a mass 1.226 greater than Venus, should have had 5.01020 kg of CO2. If entirely precipitated as carbonate, the Earth should now have 1.11021 kg of carbonate. A recent estimate (Hay, 1985) gives the total volume of carbonate rock on Earth as 276.1106 km3 which, for an average density of 2.83, corresponds to a mass of 7.81020 kg. This figure and the ratio limestone/shale/sandstone of 15/74/11 (Garrels &Mackenzie, 1971) leads to the carbonate inventory shown in Table 1.
    Type of Medium: Electronic Resource
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