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Titlebook: Origin of Life; Proceedings of the T Yecheskel Wolman Conference proceedings 1981 D. Reidel Publishing Company, Dordrecht, Holland 1981 Cam

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书目名称Origin of Life
副标题Proceedings of the T
编辑Yecheskel Wolman
视频video
图书封面Titlebook: Origin of Life; Proceedings of the T Yecheskel Wolman Conference proceedings 1981 D. Reidel Publishing Company, Dordrecht, Holland 1981 Cam
描述This volume is a record of the 6th International Conference on the Origins of Life and the 3rd Meeting of the International Society for the Study of the Origins of Life. The conference was held under the auspices of the Israel Academy of Sciences and Humanities at Jerusalem from June 22nd to June 27th 1980. A few weeks prior to the conference, Academician Aleksander Ivanovich Oparin passed away. Oparin, the father and founder of the study of the origins of life, proposed over 50 years ago that modern biological molecules had abidogical origins in the past, thus the beginning of life on Earth was preceded by a long period of abiogenic molecular evolution. Oparin was planning to report on his latest work in the opening session of the meeting - "Natural Selection: A Leading Factor in Transition from the Non-Living Matter to Life". This lecture will never be delivered. In Hebrew we say of those who have died "may their memory be bound with the bonds of eternal life". For Aleksander Ivanovich Oparin those words have particular significance, for surely his pioneering work will endure as long as the spirit of scientific enquiry prevails. This meeting was dedicated to the memory of Aleksan
出版日期Conference proceedings 1981
关键词Cambrian; Cloud; Halophile; Phanerozoic; adsorption; atmosphere; bacteria; clays; energy; formation; metabolis
版次1
doihttps://doi.org/10.1007/978-94-009-8420-2
isbn_softcover978-94-009-8422-6
isbn_ebook978-94-009-8420-2
copyrightD. Reidel Publishing Company, Dordrecht, Holland 1981
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On the Origin of Organic Molecules in Interstellar Space and Some of its Consequences,s cannot possibly explain the observed amounts of complex organic molecules. They are probably formed in interstellar clouds, either free in space or on the surface of grains. This opens the possibility that planets (also the earth) moving through such clouds may have collected appreciable amounts o
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Nature and Origin of Organic Molecules in Comets,lar grains that have later accreted into comets, or they represent the “snows” that condensed onto silicate grains during the cooling phase of the presolar nebula. Even if one does not accept the speculations of Hoyle and Wickramashinghe (1977), the fact that prebiotic chemistry could have been brou
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Liquid Water on a Planet over Cosmic Periods,se effect of the planet, if not properly compensated, can elliminate liquid water from the surface of the planet either through runaway glaciation or through a runaway greenhouse effect. Since active life, at least as we know it, requires the presence of liquid water, and since its evolution to high
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Nitrogen Compounds in Carbonaceous Meteorites: A Reassessment,laboratory. The positive identification of the pyrimidine uracil and the purines adenine, guanine, xanthine and hypoxanthine is reported. The .-triazines melamine, ammeline, ammelide and cyanuric acid could not be detected in any meteorite, above a detection limit of 50 ppb.
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