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Titlebook: Astronomical Origins of Life; Steps Towards Panspe F. Hoyle,N. C. Wickramasinghe Book 2000 Springer Science+Business Media Dordrecht 2000 G

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期刊全称Astronomical Origins of Life
期刊简称Steps Towards Panspe
影响因子2023F. Hoyle,N. C. Wickramasinghe
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图书封面Titlebook: Astronomical Origins of Life; Steps Towards Panspe F. Hoyle,N. C. Wickramasinghe Book 2000 Springer Science+Business Media Dordrecht 2000 G
影响因子Living material contains about twenty different sorts of atom combined into a set of relatively simple molecules. Astrobiologists tend to believe that abiotic mater­ ial will give rise to life in any place where these molecules exist in appreciable abundances and where physical conditions approximate to those occurring here on Earth. We think this popular view is wrong, for it is not the existence of the building blocks of life that is crucial but the exceedingly complicated structures in which they are arranged in living forms. The probability of arriving at biologically significant arrangements is so very small that only by calling on the resources of the whole universe does there seem to be any possibility of life originating, a conclusion that requires life on the Earth to be a minute component of a universal system. Some think that the hugely improbable transition from non-living to living mat­ ter can be achieved by dividing the transition into many small steps, calling on a so-called ‘evolutionary‘ process to bridge the small steps one by one. This claim turns on semantic arguments which seek to replace the probability for the whole chain by the sum of the individual probabi
Pindex Book 2000
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https://doi.org/10.1007/978-3-322-84328-9ral types of galactic infrared source. The model used in these computations involves polysaccharide condensation in material flowing out from O-type stars. With the exception of rather minor discrepancies we show that it is possible to match the 2.1-13 μ observations of a wide range of galactic infrared sources.
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Biological Activity in the Early Solar System in its Outer Regionssolar system some 4 billion years ago. The requirement of a liquid condition within comets was maintained for an initial epoch through the energy released in radioactive decays. When such energy sources eventually became exhausted inward freezing led to the production of multi-cracked, fragile cometary structures.
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