Kasting James F, Howard M Tazewell
Department of Geosciences, Penn State University, University Park, PA 16802, USA.
Philos Trans R Soc Lond B Biol Sci. 2006 Oct 29;361(1474):1733-41; discussion 1741-2. doi: 10.1098/rstb.2006.1902.
Oxygen isotope data from ancient sedimentary rocks appear to suggest that the early Earth was significantly warmer than today, with estimates of surface temperatures between 45 and 85 degrees C. We argue, following others, that this interpretation is incorrect-the same data can be explained via a change in isotopic composition of seawater with time. These changes in the isotopic composition could result from an increase in mean depth of the mid-ocean ridges caused by a decrease in geothermal heat flow with time. All this implies that the early Earth was warm, not hot.A more temperate early Earth is also easier to reconcile with the long-term glacial record. However, what triggered these early glaciations is still under debate. The Paleoproterozoic glaciations at approximately 2.4Ga were probably caused by the rise of atmospheric O2 and a concomitant decrease in greenhouse warming by CH4. Glaciation might have occurred in the Mid-Archaean as well, at approximately 2.9Ga, perhaps as a consequence of anti-greenhouse cooling by hydrocarbon haze. Both glaciations are linked to decreases in the magnitude of mass-independent sulphur isotope fractionation in ancient rocks. Studying both the oxygen and sulphur isotopic records has thus proved useful in probing the composition of the early atmosphere.
来自古代沉积岩的氧同位素数据似乎表明,早期地球比现在要温暖得多,据估计其表面温度在45到85摄氏度之间。我们赞同其他人的观点,认为这种解释是不正确的——同样的数据可以通过海水同位素组成随时间的变化来解释。同位素组成的这些变化可能是由于随着时间的推移地热能流减少导致大洋中脊平均深度增加所致。所有这些都意味着早期地球是温暖的,而非炎热的。一个更为温和的早期地球也更容易与长期的冰川记录相协调。然而,引发这些早期冰川作用的原因仍在争论之中。大约在24亿年前的古元古代冰川作用可能是由大气中氧气的增加以及随之而来的甲烷温室效应减弱所导致的。太古宙中期大约在29亿年前可能也发生过冰川作用,或许是由碳氢化合物霾造成的反温室效应冷却所致。这两次冰川作用都与古代岩石中质量无关的硫同位素分馏程度的降低有关。因此,研究氧和硫同位素记录已被证明有助于探究早期大气的组成。