Watson Andrew J
School of Environmental Science, University of East Anglia, Norwich, UK.
Astrobiology. 2008 Feb;8(1):175-85. doi: 10.1089/ast.2006.0115.
Structurally complex life and intelligence evolved late on Earth; models for the evolution of global temperature suggest that, due to the increasing solar luminosity, the future life span of the (eukaryote) biosphere will be "only" about another billion years, a short time compared to the approximately 4 Ga since life began. A simple stochastic model (Carter, 1983) suggests that this timing might be governed by the necessity to pass a small number, n, of very difficult evolutionary steps, with n < 10 and a best guess of n = 4, in order for intelligent observers like ourselves to evolve. Here I extend the model analysis to derive probability distributions for each step. Past steps should tend to be evenly spaced through Earth's history, and this is consistent with identification of the steps with some of the major transitions in the evolution of life on Earth. A complementary approach, identifying the critical steps with major reorganizations in Earth's biogeochemical cycles, suggests that the Archean-Proterozoic and Proterozoic-Phanerozoic transitions might be identified with critical steps. The success of the model lends support to a "Rare Earth" hypothesis (Ward and Brownlee, 2000): structurally complex life is separated from prokaryotes by several very unlikely steps and, hence, will be much less common than prokaryotes. Intelligence is one further unlikely step, so it is much less common still.
结构复杂的生命和智能在地球历史后期才得以演化;全球气温演化模型表明,由于太阳光度不断增加,(真核生物)生物圈未来的寿命“仅”约为10亿年,与生命起源以来大约40亿年相比,这是一段短暂的时间。一个简单的随机模型(卡特,1983年)表明,这一时间安排可能受必须跨越少量(n个)非常困难的进化步骤所支配,其中n < 10,最佳猜测值为n = 4,以便像我们这样的智能观察者得以进化。在此,我扩展模型分析以得出每个步骤的概率分布。过去的步骤在地球历史中应倾向于均匀分布,这与将这些步骤与地球上生命演化的一些主要转变相识别是一致的。一种互补的方法,即将关键步骤与地球生物地球化学循环的重大重组相识别,表明太古宙 - 元古宙和元古宙 - 显生宙的转变可能与关键步骤相关。该模型的成功为“稀有地球”假说(沃德和布朗利,2000年)提供了支持:结构复杂的生命与原核生物之间隔着几个极不可能发生的步骤,因此,其出现的频率将远低于原核生物。智能是更进一步的一个不太可能发生的步骤,所以其出现的频率更低。