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The Physical, Chemical and Physiological Limits of Life

Life on Earth displays an incredible diversity in form and function, which allows it to survive not only physical extremes, but also periods of time when it is exposed to non-habitable conditions. Extreme physiological adaptations to bridge non-habitable conditions include various dormant states, su...

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Detalles Bibliográficos
Autores principales: Schulze-Makuch, Dirk, Schulze-Makuch, Alexander, Houtkooper, Joop M.
Formato: Online Artículo Texto
Lenguaje:English
Publicado: MDPI 2015
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4598648/
https://www.ncbi.nlm.nih.gov/pubmed/26193325
http://dx.doi.org/10.3390/life5031472
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author Schulze-Makuch, Dirk
Schulze-Makuch, Alexander
Houtkooper, Joop M.
author_facet Schulze-Makuch, Dirk
Schulze-Makuch, Alexander
Houtkooper, Joop M.
author_sort Schulze-Makuch, Dirk
collection PubMed
description Life on Earth displays an incredible diversity in form and function, which allows it to survive not only physical extremes, but also periods of time when it is exposed to non-habitable conditions. Extreme physiological adaptations to bridge non-habitable conditions include various dormant states, such as spores or tuns. Here, we advance the hypothesis that if the environmental conditions are different on some other planetary body, a deviating biochemistry would evolve with types of adaptations that would manifest themselves with different physical and chemical limits of life. In this paper, we discuss two specific examples: putative life on a Mars-type planet with a hydrogen peroxide-water solvent and putative life on a Titan-type planetary body with liquid hydrocarbons as a solvent. Both examples would have the result of extending the habitable envelope of life in the universe.
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spelling pubmed-45986482015-10-15 The Physical, Chemical and Physiological Limits of Life Schulze-Makuch, Dirk Schulze-Makuch, Alexander Houtkooper, Joop M. Life (Basel) Hypothesis Life on Earth displays an incredible diversity in form and function, which allows it to survive not only physical extremes, but also periods of time when it is exposed to non-habitable conditions. Extreme physiological adaptations to bridge non-habitable conditions include various dormant states, such as spores or tuns. Here, we advance the hypothesis that if the environmental conditions are different on some other planetary body, a deviating biochemistry would evolve with types of adaptations that would manifest themselves with different physical and chemical limits of life. In this paper, we discuss two specific examples: putative life on a Mars-type planet with a hydrogen peroxide-water solvent and putative life on a Titan-type planetary body with liquid hydrocarbons as a solvent. Both examples would have the result of extending the habitable envelope of life in the universe. MDPI 2015-07-17 /pmc/articles/PMC4598648/ /pubmed/26193325 http://dx.doi.org/10.3390/life5031472 Text en © 2015 by the authors; licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution license (http://creativecommons.org/licenses/by/4.0/).
spellingShingle Hypothesis
Schulze-Makuch, Dirk
Schulze-Makuch, Alexander
Houtkooper, Joop M.
The Physical, Chemical and Physiological Limits of Life
title The Physical, Chemical and Physiological Limits of Life
title_full The Physical, Chemical and Physiological Limits of Life
title_fullStr The Physical, Chemical and Physiological Limits of Life
title_full_unstemmed The Physical, Chemical and Physiological Limits of Life
title_short The Physical, Chemical and Physiological Limits of Life
title_sort physical, chemical and physiological limits of life
topic Hypothesis
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4598648/
https://www.ncbi.nlm.nih.gov/pubmed/26193325
http://dx.doi.org/10.3390/life5031472
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