Whittet D C
Department of Physics, Applied Physics and Astronomy, Rensselaer Polytechnic Institute, Troy, NY 12180, USA.
Orig Life Evol Biosph. 1997 Jun;27(1-3):249-62.
I review the relative importance of internal and external sources of prebiotic molecules on Earth at the time of life's origin approximately 3.7 Gyr ago. The efficiency of synthesis in the Earth's atmosphere was critically dependent on its oxidation state. If the early atmosphere was non-reducing and CO2-dominated, external delivery might have been the dominant source. Interplanetary dust grains and micrometeorites currently deliver carbonaceous matter to the Earth's surface at a rate of approximately 3 x 10(5) kg/yr (equivalent to a biomass in approximately 2 Gyr), but this may have been as high as 5 x 10(7) kg/yr (a biomass in only approximately 10 Myr) during the epoch of late bombardment. Much of the incoming material is in the form of chemically inactive kerogens and amorphous carbon; but if the Earth once had a dense (approximately 10-bar) atmosphere, small comets rich in a variety of prebiotic molecules may have been sufficiently air-braked to land non-destructively. Lingering uncertainties regarding the impact history of the Earth and the density and composition of its early atmosphere limit our ability to draw firm conclusions.
我回顾了大约37亿年前生命起源时地球上益生元分子的内部和外部来源的相对重要性。地球大气中合成的效率严重依赖于其氧化态。如果早期大气是非还原性的且以二氧化碳为主,那么外部输送可能是主要来源。目前,行星际尘埃颗粒和微陨石以大约每年3×10⁵千克的速率将含碳物质输送到地球表面(相当于大约20亿年中的生物量),但在晚期重轰炸时期,这一速率可能高达每年5×10⁷千克(仅约1000万年中的生物量)。大部分进入的物质是以化学惰性的干酪根和无定形碳的形式存在;但如果地球曾经有一个浓密(约10巴)的大气,富含各种益生元分子的小彗星可能会受到足够的空气制动而无损着陆。关于地球撞击历史以及其早期大气密度和组成的不确定性仍然存在,这限制了我们得出确凿结论的能力。