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When did oxygenic photosynthesis evolve?

机译:氧气的光合作用何时开始发展?

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The atmosphere has apparently been oxygenated since the ‘Great Oxidation Event’ ca 2.4Ga ago, but when the photosynthetic oxygen production began is debatable. However, geological and geochemical evidence from older sedimentary rocks indicates that oxygenic photosynthesis evolved well before this oxygenation event. Fluid-inclusion oils in ca 2.45Ga sandstones contain hydrocarbon biomarkers evidently sourced from similarly ancient kerogen, preserved without subsequent contamination, and derived from organisms producing and requiring molecular oxygen. Mo and Re abundances and sulphur isotope systematics of slightly older (2.5Ga) kerogenous shales record a transient pulse of atmospheric oxygen. As early as ca 2.7Ga, stromatolites and biomarkers from evaporative lake sediments deficient in exogenous reducing power strongly imply that oxygen-producing cyanobacteria had already evolved. Even at ca 3.2Ga, thick and widespread kerogenous shales are consistent with aerobic photoautrophic marine plankton, and U–Pb data from ca 3.8Ga metasediments suggest that this metabolism could have arisen by the start of the geological record. Hence, the hypothesis that oxygenic photosynthesis evolved well before the atmosphere became permanently oxygenated seems well supported.
机译:自从大约2.4Ga发生“重大氧化事件”以来,大气显然已被充氧,但是光合氧气的产生开始时尚有争议。然而,来自较老沉积岩的地质和地球化学证据表明,氧的光合作用在此氧化事件发生之前就已经发生了。大约2.45Ga砂岩中的流体包裹体油含有烃类生物标志物,这些烃类标志物显然来自相似的古代干酪根,保存后未受到任何污染,并来源于产生并需要分子氧的生物。年龄稍长的(2.5Ga)干酪根页岩的Mo和Re丰度以及硫同位素系统记录了大气氧的瞬时脉冲。早在ca 2.7Ga时,缺乏外源还原能力的蒸发湖沉积物中的叠层石和生物标志物就强烈暗示了已经产生了产氧的蓝细菌。即使在约3.2Ga处,厚厚且广泛的干酪根页岩也与有氧光合营养性海洋浮游生物一致,并且约3.8Ga沉积物的U-Pb数据表明这种代谢可能是在地质记录开始时就已经发生的。因此,氧的光合作用在大气被永久性氧化之前就已经充分发展的假说似乎得到了很好的支持。

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