首页> 外文OA文献 >The Effects of Parent Body Processes on Amino Acids in Carbonaceous Chondrites
【2h】

The Effects of Parent Body Processes on Amino Acids in Carbonaceous Chondrites

机译:母体过程对碳质球粒陨石中氨基酸的影响

代理获取
本网站仅为用户提供外文OA文献查询和代理获取服务,本网站没有原文。下单后我们将采用程序或人工为您竭诚获取高质量的原文,但由于OA文献来源多样且变更频繁,仍可能出现获取不到、文献不完整或与标题不符等情况,如果获取不到我们将提供退款服务。请知悉。

摘要

To investigate the effect of parent body processes on the abundance, distribution, and enantiomeric composition of amino acids in carbonaceous chondrites, the water extracts from nine different powdered Cl, CM, and CR carbonaceous chondrites were analyzed for amino acids by ultrahigh performance liquid chromatography-fluorescence detection and time-of-flight mass spectrometry (UPLC-FD/ToF-MS). Four aqueously altered type 1 carbonaceous chondrites including Orgueil (C11), Meteorite Hills (MET) 01070 (CM1), Scott Glacier (SCO) 06043 (CM1), and Grosvenor Mountains (GRO) 95577 (CR1) were analyzed using this technique for the first time. Analyses of these meteorites revealed low levels of two- to five-carbon acyclic amino alkanoic acids with concentrations ranging from -1 to 2,700 parts-per-billion (ppb). The type 1 carbonaceous chondrites have a distinct distribution of the five-carbon (C5) amino acids with much higher relative abundances of the gamma- and delta-amino acids compared to the type 2 and type 3 carbonaceous chondrites, which are dominated by a-amino acids. Much higher amino acid abundances were found in the CM2 chondrites Murchison, Lonewolf Nunataks (LON) 94102, and Lewis Cliffs (LEW) 90500, the CR2 Elephant Moraine (EET) 92042, and the CR3 Queen Alexandra Range (QUE) 99177. For example, a-aminoisobutyric acid ((alpha-AIB) and isovaline were approximately 100 to 1000 times more abundant in the type 2 and 3 chondrites compared to the more aqueously altered type 1 chondrites. Most of the chiral amino acids identified in these meteorites were racemic, indicating an extraterrestrial abiotic origin. However, non-racemic isovaline was observed in the aqueously altered carbonaceous chondrites Murchison, Orgueil, SCO 06043, and GRO 95577 with L-isovaline excesses ranging from approximately 11 to 19%, whereas the most pristine, unaltered carbonaceous chondrites analyzed in this study had no detectable L-isovaline excesses. These results are consistent with the theory that aqueous alteration played an important role in amplification of small initial left handed isovaline excesses on the parent bodies.
机译:为了研究母体过程对碳质球粒陨石中氨基酸含量,分布和对映体组成的影响,通过超高效液相色谱法分析了9种不同粉状Cl,CM和CR碳质球粒陨石中水提取物的氨基酸含量,荧光检测和飞行时间质谱(UPLC-FD / ToF-MS)。使用此技术分析了四种含水改变的1型碳质球粒陨石,包括Orgueil(C11),Meteorite Hills(MET)01070(CM1),Scott Glacier(SCO)06043(CM1)和Grosvenor Mountains(GRO)95577(CR1)。第一次。对这些陨石的分析显示,低浓度的2至5个碳原子的无环氨基链烷酸的浓度范围为-1至2,700十亿分之一(ppb)。与2型和3型碳质球粒陨石相比,1型碳质球粒陨石具有明显不同的五碳(C5)氨基酸分布,γ-和δ-氨基酸的相对丰度要高得多。氨基酸。在CM2球粒陨石Murchison,Lonewolf Nunataks(LON)94102和Lewis Cliffs(LEW)90500,CR2 Elephant Moraine(EET)92042和CR3 Queen Alexandra Range(QUE)99177中发现了更高的氨基酸丰度。 ,α-氨基异丁酸((α-AIB)和异戊酸在2型和3型球粒陨石中的含量大约是水变的1型球粒陨石的大约100到1000倍。在这些陨石中鉴定出的大多数手性氨基酸是外消旋的,这表明是外星生物的起源。然而,在含水改变的碳质球粒体Murchison,Orgueil,SCO 06043和GRO 95577中观察到非外消旋异缬氨酸,其中L-异缬氨酸过量的范围约为11%至19%,而最原始的未改变这项研究中分析的碳质球粒陨石没有可检测到的L-异缬氨酸过量,这些结果与以下理论相一致:水相蚀变在小分子起始放大中起重要作用母体上所有左手异戊酸过量。

著录项

相似文献

  • 外文文献
  • 中文文献
  • 专利
代理获取

客服邮箱:kefu@zhangqiaokeyan.com

京公网安备:11010802029741号 ICP备案号:京ICP备15016152号-6 六维联合信息科技 (北京) 有限公司©版权所有
  • 客服微信

  • 服务号