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Titlebook: Strategies for the Search for Life in the Universe; A Joint Session of C Michael D. Papagiannis Book 1980 D. Reidel Publishing Company, Dor

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發(fā)表于 2025-3-23 10:44:27 | 只看該作者
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發(fā)表于 2025-3-23 14:35:59 | 只看該作者
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發(fā)表于 2025-3-23 19:32:47 | 只看該作者
N is Neither Very Small nor Very Large is not supported observationally. The suggestion that the lack of extraterrestrial colonists on the earth means that N is very small is examined in detail. It is shown that the interstellar colonization scenario is, in fact, not plausible because even one colony calls for expenditures of energy suf
14#
發(fā)表于 2025-3-24 00:09:50 | 只看該作者
Galactic-Scale Civilization evolution, social evolution, and cultural evolution. In this process, matter becomes organized in increasingly complex ways, and more able to make use of free energy in the environment. In view of this evolution of dissipative structures, of which cells, humans, and mankind are examples, it seems u
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發(fā)表于 2025-3-24 05:10:47 | 只看該作者
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發(fā)表于 2025-3-24 10:03:35 | 只看該作者
Uncertainty in Estimates of the Number of Extraterrestrial Civilizations to some extent uncertain. The uncertainty in any quantity may be represented by a probability distribution function, even if that quantity is itself a probability. The uncertainty of current estimates of N is derived principally from uncertainty in estimates of the lifetime of advanced civilization
17#
發(fā)表于 2025-3-24 14:26:32 | 只看該作者
Strategies for SETI Through Radio Waves an Introductionwould have been colonized or at least visited long ago. Of course, followers of Von D?niken believe we . been, while the UFO buffs believe we are . being visited. But a more skeptical faction, finding no solid evidence either for visitation or for astro-engineering on a Dyson scale, concludes that e
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發(fā)表于 2025-3-24 16:17:45 | 只看該作者
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發(fā)表于 2025-3-24 20:51:15 | 只看該作者
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發(fā)表于 2025-3-24 23:17:10 | 只看該作者
Search for Planets and Early Life in Other Solar Systems an Introductionmental importance to the question of life, because we assume that life may originate and evolve only on planets. If planets were found near other stars, then with the development of proper instruments we could go one step further and search for a spectroscopic evidence of early life on these planets
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