Greenberg J M, Mendoza-Gomez C X
Department of Astronomy and Physics, Leiden University, The Netherlands.
Adv Space Res. 1992;12(4):169-80. doi: 10.1016/0273-1177(92)90170-3.
The evidence that living organisms were already extant on the earth almost 4 Gyr ago and that early bombardment by comets and asteroids created a hostile environment up to about this time has revived the question of how it was possible for prebiotic chemical evolution to have provided the necessary ingredients for life to have developed in the short intervening time. The actual bracketed available temporal space is no more than 0.5 Gyr and probably much less. Was this sufficient time for an earth-based source of the first simple organic precursor molecules to have led to the level of the prokaryotic cell? If not, then the difficulty would be resolved if the ancient earth was impregnated by organic molecular seed from outer space. Curiously, it seems that the most likely source of such seeds was the same a one of the sources of the hostile enviroment, namely the comets which bombarded the earth. With the knowledge of comets gained by the space missions it has become clear that a very large fraction of the chemical composition of comet nuclei consists of quite complex organic molecules. Furthermore it has been demonstrated that comets consist of very fluffy aggregates of interstellar dust whose chemistry derives from photoprocessing of simple ice mixtures in space. Thus, the ultimate source of organics in comets comes from the chemical evolution of interstellar dust. An important and critical justification for assuming that interstellar dust is the ultimate source of prebiotic molecular insertion on the earth is the proof that comets are extremely fluffy aggregates, which have the possibility of breaking up into finely divided fragments when the comet impacts the earth's atmosphere. In the following we will summarize the properties of interstellar dust and the chemical and morphological structure of comets indicated by the most recent interpretations of comet observations. It will be shown that the suitable condition for comets having provided abundant prebiotic molecules as well as the water in which they could have further evolved are consistent with theories of the early earth environment.
有证据表明,地球上在近40亿年前就已存在生物,并且直到大约这个时期,彗星和小行星的早期撞击都创造了一个恶劣的环境,这再次引发了一个问题:在前生物化学进化过程中,如何有可能在如此短暂的时间内提供生命发展所需的必要成分。实际可用的时间跨度不超过5亿年,可能还要少得多。这段时间是否足以让地球上的第一个简单有机前体分子来源发展到原核细胞的水平呢?如果不够,那么如果古代地球被来自外太空的有机分子种子所渗透,这个难题就会得到解决。奇怪的是,这种种子最有可能的来源似乎与恶劣环境的来源之一相同,即撞击地球的彗星。随着太空任务对彗星的了解,很明显彗星核的很大一部分化学成分由相当复杂的有机分子组成。此外,已经证明彗星由非常蓬松的星际尘埃聚集体组成,其化学性质源于太空中简单冰混合物的光处理。因此,彗星中有机物的最终来源来自星际尘埃的化学进化。假设星际尘埃是地球上前生物分子插入的最终来源的一个重要且关键的理由是,有证据表明彗星是极其蓬松的聚集体,当彗星撞击地球大气层时,有可能分裂成细小的碎片。在下面,我们将总结星际尘埃的特性以及根据对彗星观测的最新解释所表明的彗星的化学和形态结构。结果将表明,彗星提供丰富的前生物分子以及它们可以进一步进化的水的适宜条件与早期地球环境的理论是一致的。