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Detectability of life and photosynthesis on exoplanets

机译:系外行星生命和光合作用的可检测性

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‘Is there life on exoplanets?’. We refer to exoplanets as planets in other solar systems than our own. This often asked question can be further refined by asking ‘is there life on exoplanets which is so extensive that it may impact on its atmosphere, its biosphere and its optical properties?’. And if such a life exists, at astronomical distances from us, can we detect it with instruments on Earth-based or Earth-orbiting observatories? Will then, in that case, our advanced knowledge of present-dayand early-day photosynthesis on Earth help usselect appropriate biosignatures that may signal its presence? Here we elaborate further on these themes,based on the most recent literature, and from the point of view of photosynthesis. We also provide our consideredviews. Although search for chlorophyll is considered desirable, we conclude that our best bet is tolook for and analyse photosynthesis-related gases, namely O_2, CO_2 and H2O vapour. We shall keep in mindthat the evolutionary tree of life on our planet has its roots in autotrophy, and of the various forms of autotrophy, only oxygenic photosynthesis can produce massive amounts of reduced carbon and free O2, both inwater and on land.
机译:“系外行星上有生命吗?”。我们称系外行星是我们太阳系以外其他太阳系中的行星。这个常见问题可以通过询问“系外行星上是否存在如此广泛的生命,从而可能影响其大气,生物圈及其光学特性?”来进一步完善。如果存在这样的生命,并且距离我们天文距离遥远,我们是否可以在地基或地球轨道观测站上用仪器检测到它?那么,在那种情况下,我们在地球上当今和早期的光合作用方面的先进知识是否可以帮助我们选择可能预示其存在的适当生物特征?在此,我们基于最新文献并从光合作用的角度进一步阐述这些主题。我们还提供了我们的意见。尽管寻找叶绿素被认为是可取的,但我们得出的结论是,最好的选择是寻找和分析与光合作用相关的气体,即O_2,CO_2和H2O蒸气。我们将牢记,我们星球上的进化生命树源于自养,而自养的形式多种多样,只有氧的光合作用才能在水中和陆地上产生大量的还原碳和游离O2。

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