Matthews C N, Ludicky R
Department of Chemistry, University of Illinois at Chicago 60680, USA.
Adv Space Res. 1992;12(4):21-32. doi: 10.1016/0273-1177(92)90149-r.
The original presence on cometary nuclei of frozen volatiles such as methane, ammonia and water makes them ideal sites for the formation and condensed-phase polymerization of hydrogen cyanide. We propose that the non-volatile black crust of comet Halley consists largely of such polymers. Dust emanating from Halley's nucleus, contributing to the coma and tail, would also arise partly from these solids. Indeed, secondary species such as CN have been widely detected, as well as HCN itself and particles consisting only of H, C and N. Our continuing investigations suggest that the yellow-orange-brown-black polymers are of two types: ladder structures with conjugated -C=N- bonds, and polyamidines readily converted by water to polypeptides. These easily formed macromolecules could be major components of the dark matter observed on the giant planets Jupiter and Saturn, as well as on outer solar system bodies such as asteroids, moons and other comets. Implications for prebiotic chemistry are profound. Primitive Earth may have been covered by HCN polymers either through cometary bombardment or by terrestrial happenings of the kind that brought about the black crust of Halley. The resulting proteinaceous matrix could have promoted the molecular interactions leading to the emergence of life.
彗星核上原本存在的甲烷、氨和水等冷冻挥发物,使其成为氰化氢形成和凝聚相聚合的理想场所。我们认为,哈雷彗星的不挥发黑色外壳主要由这类聚合物组成。从哈雷彗星核散发出来、形成彗发和彗尾的尘埃,也部分源自这些固体物质。事实上,诸如CN等次生物质以及HCN本身和仅由H、C和N组成的粒子已被广泛探测到。我们持续的研究表明,这些黄橙棕黑色聚合物有两种类型:具有共轭-C=N-键的梯形结构,以及易被水转化为多肽的聚脒。这些易于形成的大分子可能是在木星和土星等巨行星以及小行星、卫星和其他彗星等外太阳系天体上观测到的暗物质的主要成分。这对生命起源前的化学有着深远的影响。原始地球可能通过彗星撞击或类似导致哈雷彗星黑色外壳形成的地球事件,被HCN聚合物覆盖。由此产生的蛋白质基质可能促进了导致生命出现的分子相互作用。