Cronin J R, Pizzarello S
Department of Chemistry, Arizona State University, Tempe 85287, USA.
Geochim Cosmochim Acta. 1986;50:2419-27. doi: 10.1016/0016-7037(86)90024-4.
All of the eighteen possible seven-carbon acyclic primary alpha-amino alkanoic acids have been positively identified in a hot-water extract of the Murchison meteorite by the combined use of gas chromatography-mass spectrometry, ion exchange chromatography and reversed-phase chromatography. None of these amino acids has previously been found in meteorites or in any other natural material. They range in concentration from < or = 0.5 to 5.3 nmol g-1. Configuration assignments were made for 2-amino-3,4-dimethylpentanoic acid and allo-2-amino-3,4-dimethylpenatonoic acid and the diasteromer ratio was determined. Fifty-five amino acids have now been positively identified in the Murchison meteorite, 36 of which are unknown in terrestrial materials. This unique suite of amino acids is characterized by the occurrence of all structural isomers within the two major classes of amino acids represented, by the predominance of branched chain isomers, and by an exponential decline in amount with increasing carbon chain length within homologous series. These characteristics of the Murchison amino acids are suggestive of synthesis before incorporation into a parent body.
通过气相色谱-质谱联用、离子交换色谱和反相色谱等方法,在默奇森陨石的热水提取物中已明确鉴定出所有18种可能的七碳无环伯α-氨基链烷酸。这些氨基酸此前从未在陨石或任何其他天然物质中被发现过。它们的浓度范围为≤0.5至5.3 nmol g-1。已对2-氨基-3,4-二甲基戊酸和别-2-氨基-3,4-二甲基戊酸进行了构型归属,并确定了非对映体比例。目前已在默奇森陨石中明确鉴定出55种氨基酸,其中36种在地球物质中是未知的。这套独特的氨基酸具有以下特点:在代表的两类主要氨基酸中存在所有结构异构体,支链异构体占优势,并且在同系物系列中随着碳链长度增加数量呈指数下降。默奇森陨石氨基酸的这些特征表明它们是在并入母体之前合成的。