Department of Astronomy, Columbia University, New York, New York.
Astrobiology. 2018 Dec;18(12):1574-1584. doi: 10.1089/ast.2018.1836. Epub 2018 Oct 31.
Life appears to have emerged relatively quickly on the Earth, a fact sometimes used to justify a high rate of spontaneous abiogenesis () among Earth-like worlds. Conditioned upon a single datum-the time of earliest evidence for life ()-previous Bayesian formalisms for the posterior distribution of have demonstrated how inferences are highly sensitive to the priors. Rather than attempt to infer the true posterior, we here compute the relative change to when new experimental/observational evidence is introduced. By simulating posterior distributions and resulting entropic information gains, we compare three experimental pressures on : (1) evidence for an earlier start to life, , (2) constraints on spontaneous abiogenesis from the laboratory, and (3) an exoplanet survey for biosignatures. First, we find that experiments 1 and 2 can only yield lower limits on , unlike 3. Second, evidence for an earlier start to life can yield negligible information on if [Formula: see text]. Vice versa, experiment 2 is uninformative when [Formula: see text]. While experiment 3 appears the most direct means of measuring , we highlight that early starts inform us of the conditions of abiogenesis and that laboratory experiments could succeed in building new life. Altogether, the three experiments are complementary, and we encourage activity in all to solve this grand challenge.
生命似乎在地球上迅速出现,这一事实有时被用来证明类似地球的世界中自发的生物起源率很高。基于最早生命证据的时间()这一个数据,先前用于推断的贝叶斯形式主义表明了这些推断对先验的高度敏感性。我们不是试图推断真正的后验,而是在这里计算当引入新的实验/观测证据时对的相对变化。通过模拟后验分布和由此产生的熵信息增益,我们比较了对的三种实验压力:(1)生命开始更早的证据,(2)来自实验室的自发生物起源的限制,以及(3)系外行星生物特征调查。首先,我们发现实验 1 和 2 只能对给出下界,而不像实验 3 那样。其次,如果[公式:见正文],那么生命开始更早的证据对的信息增益可以忽略不计。相反,当[公式:见正文]时,实验 2 是没有信息量的。虽然实验 3 似乎是测量的最直接手段,但我们强调早期开始可以为生物起源的条件提供信息,并且实验室实验可能成功地构建新的生命。总之,这三个实验是互补的,我们鼓励所有这些实验的活动,以解决这一重大挑战。