Department of Natural History, Royal Ontario Museum, Toronto, ON M5S 2C6, Canada;
Department of Earth Sciences, University of Toronto, Toronto, ON M5S 3B1, Canada.
Proc Natl Acad Sci U S A. 2020 May 26;117(21):11217-11219. doi: 10.1073/pnas.2003276117. Epub 2020 May 11.
Understanding the timing and mechanisms of amino acid synthesis and racemization on asteroidal parent bodies is key to demonstrating how amino acids evolved to be mostly left-handed in living organisms on Earth. It has been postulated that racemization can occur rapidly dependent on several factors, including the pH of the aqueous solution. Here, we conduct nanoscale geochemical analysis of a framboidal magnetite grain within the Tagish Lake carbonaceous chondrite to demonstrate that the interlocking crystal arrangement formed within a sodium-rich, alkaline fluid environment. Notably, we report on the discovery of Na-enriched subgrain boundaries and nanometer-scale Ca and Mg layers surrounding individual framboids. These interstitial coatings would yield a surface charge state of zero in more-alkaline fluids and prevent assimilation of the individual framboids into a single grain. This basic solution would support rapid synthesis and racemization rates on the order of years, suggesting that the low abundances of amino acids in Tagish Lake cannot be ascribed to fluid chemistry.
了解氨基酸在小行星母体上的合成和外消旋作用的时间和机制是证明氨基酸在地球上的生命体中如何进化为主要左旋的关键。据推测,外消旋作用的发生速度取决于几个因素,包括水相溶液的 pH 值。在这里,我们对来自塔吉什湖碳质球粒陨石中的一个莓球状磁铁矿颗粒进行了纳米级地球化学分析,以证明在富含钠的碱性流体环境中形成了互锁的晶体排列。值得注意的是,我们报告了在单个莓球状颗粒周围发现了富含钠的亚晶粒边界和纳米级钙和镁层。这些间隙涂层在更碱性的流体中会产生零表面电荷状态,并防止单个莓球状颗粒聚集成单个晶粒。这种基本溶液可以支持在数年时间尺度内快速合成和外消旋,这表明塔吉什湖低丰度的氨基酸不能归因于流体化学。