Liebman S A, Pesce-Rodriguez R A, Matthews C N
CCS Instrument Systems, Inc., Avondale, PA 19311, USA.
Adv Space Res. 1995 Mar;15(3):71-80. doi: 10.1016/s0273-1177(99)80066-0.
Hydrogen cyanide polymerizes readily to a black solid from which a yellow-brown powder can be extracted by water and further hydrolyzed to alpha-amino acids. These macromolecules could be major components of the dark matter observed on many bodies in the outer solar system, including comets and asteroids. Primitive Earth might therefore have been covered with HCN polymers through bolide bombardment or be terrestrial synthesis. Several instrumental methods were used for the separation and identification of these intriguing polymeric materials, including photoacoustic Fourier transform infrared spectroscopy, supercritical fluid extraction chromatography and pyrolysis mass spectrometry. Our integrated analytical approach revealed fragmentation patterns and chemical functionalities consistent with the presence of polymeric peptide precursors both in HCN polymers and in the Murchison meteorite.
氰化氢很容易聚合成黑色固体,用水可以从中提取出黄褐色粉末,并进一步水解为α-氨基酸。这些大分子可能是在外太阳系许多天体(包括彗星和小行星)上观测到的暗物质的主要成分。因此,原始地球可能通过火流星撞击或陆地合成而被氰化氢聚合物覆盖。几种仪器方法被用于分离和鉴定这些有趣的聚合材料,包括光声傅里叶变换红外光谱法、超临界流体萃取色谱法和热解质谱法。我们的综合分析方法揭示了与氰化氢聚合物和默奇森陨石中聚合肽前体的存在相一致的碎片模式和化学官能团。