Levy M, Miller S L, Brinton K, Bada J L
Department of Chemistry, University of California, San Diego, La Jolla 92093-0506, USA.
Icarus. 2000 Jun;145(2):609-13. doi: 10.1006/icar.2000.6365.
In order to simulate prebiotic synthetic processes on Europa and other ice-covered planets and satellites, we have investigated the prebiotic synthesis of organic compounds from dilute solutions of NH4CN frozen for 25 years at -20 and -78 degrees C. In addition, the aqueous products of spark discharge reactions from a reducing atmosphere were frozen for 5 years at -20 degrees C. We find that both adenine and guanine, as well as a simple set of amino acids dominated by glycine, are produced in substantial yields under these conditions. These results indicate that some of the key components necessary for the origin of life may have been available on Europa throughout its history and suggest that the circumstellar zone where life might arise may be wider than previously thought.
为了模拟木卫二及其他冰封行星和卫星上的益生元合成过程,我们研究了在-20℃和-78℃下冷冻25年的NH4CN稀溶液中有机化合物的益生元合成。此外,将还原性气氛中火花放电反应的水相产物在-20℃下冷冻5年。我们发现,在这些条件下,腺嘌呤和鸟嘌呤以及以甘氨酸为主的一组简单氨基酸都能大量产生。这些结果表明,生命起源所需的一些关键成分可能在木卫二的整个历史中都存在,这表明可能出现生命的星周区域可能比之前认为的更广泛。