Garcia Adrien D, Meinert Cornelia, Sugahara Haruna, Jones Nykola C, Hoffmann Søren V, Meierhenrich Uwe J
Institut de Chimie de Nice, Université Côte d'Azur, CNRS, UMR 7272, 06108 Nice, France.
Japan Aerospace Exploration Agency⁻Institute of Space and Astronautical Science, 3-1-1 Yoshinodai, Chuo Sagamihara, Kanagawa 252-5210, Japan.
Life (Basel). 2019 Mar 16;9(1):29. doi: 10.3390/life9010029.
The biomolecular homochirality in living organisms has been investigated for decades, but its origin remains poorly understood. It has been shown that circular polarized light (CPL) and other energy sources are capable of inducing small enantiomeric excesses (s) in some primary biomolecules, such as amino acids or sugars. Since the first findings of amino acids in carbonaceous meteorites, a scenario in which essential chiral biomolecules originate in space and are delivered by celestial bodies has arisen. Numerous studies have thus focused on their detection, identification, and enantiomeric excess calculations in extraterrestrial matrices. In this review we summarize the discoveries in amino acids, sugars, and organophosphorus compounds in meteorites, comets, and laboratory-simulated interstellar ices. Based on available analytical data, we also discuss their interactions with CPL in the ultraviolet (UV) and vacuum ultraviolet (VUV) regions, their abiotic chiral or achiral synthesis, and their enantiomeric distribution. Without doubt, further laboratory investigations and upcoming space missions are required to shed more light on our potential extraterrestrial molecular origins.
几十年来,人们一直在研究生物体内的生物分子同手性,但对其起源仍知之甚少。研究表明,圆偏振光(CPL)和其他能源能够在一些初级生物分子(如氨基酸或糖类)中诱导出小的对映体过量(s)。自首次在碳质陨石中发现氨基酸以来,一种基本手性生物分子起源于太空并由天体传递的设想就出现了。因此,许多研究都集中在外层空间物质中这些分子的检测、鉴定和对映体过量计算上。在这篇综述中,我们总结了在陨石、彗星和实验室模拟的星际冰中氨基酸、糖类和有机磷化合物的发现。基于现有的分析数据,我们还讨论了它们在紫外(UV)和真空紫外(VUV)区域与CPL的相互作用、它们的非生物手性或非手性合成以及它们的对映体分布。毫无疑问,需要进一步的实验室研究和即将进行的太空任务,以更深入地了解我们潜在的外星分子起源。