Abstract
“Are we alone?” or “Is Anybody Out There?” have been permanent quandaries among mankind from the ancient times to now. In this book, we are discussing the diversity of life on Earth and possibly on other celestial bodies. We always consider the phenomena of life as we know it on Earth, with the requirements for it being liquid water and carbon-based biochemistry, plus other nutrients and energy sources. In this presentation, we precluded the possibility of life as we do not know it. It is a formidable challenge to find other habitable planets or satellites, which might contain signatures of life (de Vera and Seckbach, 2013). In addition, of finding water in the search for life, we have also to search for biomolecules in our galaxy. Indeed, astrobiologists have discovered regions in our galaxy that might have the potential for producing very complex organic molecules and the starting point for the development of life. Let us examine life on Earth and compare it with some extraterrestrial conditions.
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6. Acknowledgements
The author thanks Fern Seckbach, Professors Julian Chela-Flores, David J. Chapman, and specifically Stephan Kempe for reading the text and making helpful suggestions.
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Seckbach, J. (2012). Pathways to Life on Earth and Other Planetary Bodies. In: Hanslmeier, A., Kempe, S., Seckbach, J. (eds) Life on Earth and other Planetary Bodies. Cellular Origin, Life in Extreme Habitats and Astrobiology, vol 24. Springer, Dordrecht. https://doi.org/10.1007/978-94-007-4966-5_1
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