2016
DOI: 10.4172/2332-2519.1000151
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Survival of Moss Reproductive Structures under Simulated Martian Environmental Conditions and Extreme Thermal Stress: Vibrational Spectroscopic Study and Astrobiological Implications

Abstract: The principal goal of astrobiology is the search for extraterrestrial life forms. A key aspect is the study of the ability of different kinds of terrestrial organisms to support simulated extraterrestrial environmental conditions. Mosses are multicellular green plants, poorly studied from an astrobiological perspective. In this paper, we report experimental results obtained using two species of moss, which demonstrate that both the spores of the moss Funaria hygrometrica as well as the desiccated vegetative ga… Show more

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Cited by 3 publications
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“…We have also presented evidence that the germinability of spores of the moss Funaria hygrometrica persists after exposure to simulated Martian environmental conditions inside PASC. The experimental results obtained using two species of moss, which demonstrate that both the spores of the moss Funaria hygrometrica , as well as the desiccated vegetative gametophyte shoots of the moss Tortella squarrosa ( Pleurochaete squarrosa ) were capable of resisting Simulated Martian Environmental Conditions (SMEC): Mars simulated atmospheric composition 99.9% CO 2 , and 0.6% H 2 O with a pressure of 7 mbar, 200 K and UV irradiation of 30 mW cm −2 in a wavelength range of 200–400 nm under a limited short time of exposition of two hours [83].…”
Section: Review Of Experimental Resultsmentioning
confidence: 99%
“…We have also presented evidence that the germinability of spores of the moss Funaria hygrometrica persists after exposure to simulated Martian environmental conditions inside PASC. The experimental results obtained using two species of moss, which demonstrate that both the spores of the moss Funaria hygrometrica , as well as the desiccated vegetative gametophyte shoots of the moss Tortella squarrosa ( Pleurochaete squarrosa ) were capable of resisting Simulated Martian Environmental Conditions (SMEC): Mars simulated atmospheric composition 99.9% CO 2 , and 0.6% H 2 O with a pressure of 7 mbar, 200 K and UV irradiation of 30 mW cm −2 in a wavelength range of 200–400 nm under a limited short time of exposition of two hours [83].…”
Section: Review Of Experimental Resultsmentioning
confidence: 99%