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Pressurized Martian-Like Pure CO(2) Atmosphere Supports Strong Growth of Cyanobacteria, and Causes Significant Changes in their Metabolism

Surviving of crews during future missions to Mars will depend on reliable and adequate supplies of essential life support materials, i.e. oxygen, food, clean water, and fuel. The most economical and sustainable (and in long term, the only viable) way to provide these supplies on Martian bases is via...

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Autores principales: Murukesan, Gayathri, Leino, Hannu, Mäenpää, Pirkko, Ståhle, Kurt, Raksajit, Wuttinun, Lehto, Harry J., Allahverdiyeva-Rinne, Yagut, Lehto, Kirsi
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer Netherlands 2015
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4679102/
https://www.ncbi.nlm.nih.gov/pubmed/26294358
http://dx.doi.org/10.1007/s11084-015-9458-x
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author Murukesan, Gayathri
Leino, Hannu
Mäenpää, Pirkko
Ståhle, Kurt
Raksajit, Wuttinun
Lehto, Harry J.
Allahverdiyeva-Rinne, Yagut
Lehto, Kirsi
author_facet Murukesan, Gayathri
Leino, Hannu
Mäenpää, Pirkko
Ståhle, Kurt
Raksajit, Wuttinun
Lehto, Harry J.
Allahverdiyeva-Rinne, Yagut
Lehto, Kirsi
author_sort Murukesan, Gayathri
collection PubMed
description Surviving of crews during future missions to Mars will depend on reliable and adequate supplies of essential life support materials, i.e. oxygen, food, clean water, and fuel. The most economical and sustainable (and in long term, the only viable) way to provide these supplies on Martian bases is via bio-regenerative systems, by using local resources to drive oxygenic photosynthesis. Selected cyanobacteria, grown in adequately protective containment could serve as pioneer species to produce life sustaining substrates for higher organisms. The very high (95.3 %) CO(2) content in Martian atmosphere would provide an abundant carbon source for photo-assimilation, but nitrogen would be a strongly limiting substrate for bio-assimilation in this environment, and would need to be supplemented by nitrogen fertilizing. The very high supply of carbon, with rate-limiting supply of nitrogen strongly affects the growth and the metabolic pathways of the photosynthetic organisms. Here we show that modified, Martian-like atmospheric composition (nearly 100 % CO(2)) under various low pressure conditions (starting from 50 mbar to maintain liquid water, up to 200 mbars) supports strong cellular growth. Under high CO(2) / low N(2) ratio the filamentous cyanobacteria produce significant amount of H(2) during light due to differentiation of high amount of heterocysts.
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spelling pubmed-46791022015-12-22 Pressurized Martian-Like Pure CO(2) Atmosphere Supports Strong Growth of Cyanobacteria, and Causes Significant Changes in their Metabolism Murukesan, Gayathri Leino, Hannu Mäenpää, Pirkko Ståhle, Kurt Raksajit, Wuttinun Lehto, Harry J. Allahverdiyeva-Rinne, Yagut Lehto, Kirsi Orig Life Evol Biosph Astrobiology Surviving of crews during future missions to Mars will depend on reliable and adequate supplies of essential life support materials, i.e. oxygen, food, clean water, and fuel. The most economical and sustainable (and in long term, the only viable) way to provide these supplies on Martian bases is via bio-regenerative systems, by using local resources to drive oxygenic photosynthesis. Selected cyanobacteria, grown in adequately protective containment could serve as pioneer species to produce life sustaining substrates for higher organisms. The very high (95.3 %) CO(2) content in Martian atmosphere would provide an abundant carbon source for photo-assimilation, but nitrogen would be a strongly limiting substrate for bio-assimilation in this environment, and would need to be supplemented by nitrogen fertilizing. The very high supply of carbon, with rate-limiting supply of nitrogen strongly affects the growth and the metabolic pathways of the photosynthetic organisms. Here we show that modified, Martian-like atmospheric composition (nearly 100 % CO(2)) under various low pressure conditions (starting from 50 mbar to maintain liquid water, up to 200 mbars) supports strong cellular growth. Under high CO(2) / low N(2) ratio the filamentous cyanobacteria produce significant amount of H(2) during light due to differentiation of high amount of heterocysts. Springer Netherlands 2015-08-21 2016 /pmc/articles/PMC4679102/ /pubmed/26294358 http://dx.doi.org/10.1007/s11084-015-9458-x Text en © The Author(s) 2015 Open Access This article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made.
spellingShingle Astrobiology
Murukesan, Gayathri
Leino, Hannu
Mäenpää, Pirkko
Ståhle, Kurt
Raksajit, Wuttinun
Lehto, Harry J.
Allahverdiyeva-Rinne, Yagut
Lehto, Kirsi
Pressurized Martian-Like Pure CO(2) Atmosphere Supports Strong Growth of Cyanobacteria, and Causes Significant Changes in their Metabolism
title Pressurized Martian-Like Pure CO(2) Atmosphere Supports Strong Growth of Cyanobacteria, and Causes Significant Changes in their Metabolism
title_full Pressurized Martian-Like Pure CO(2) Atmosphere Supports Strong Growth of Cyanobacteria, and Causes Significant Changes in their Metabolism
title_fullStr Pressurized Martian-Like Pure CO(2) Atmosphere Supports Strong Growth of Cyanobacteria, and Causes Significant Changes in their Metabolism
title_full_unstemmed Pressurized Martian-Like Pure CO(2) Atmosphere Supports Strong Growth of Cyanobacteria, and Causes Significant Changes in their Metabolism
title_short Pressurized Martian-Like Pure CO(2) Atmosphere Supports Strong Growth of Cyanobacteria, and Causes Significant Changes in their Metabolism
title_sort pressurized martian-like pure co(2) atmosphere supports strong growth of cyanobacteria, and causes significant changes in their metabolism
topic Astrobiology
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4679102/
https://www.ncbi.nlm.nih.gov/pubmed/26294358
http://dx.doi.org/10.1007/s11084-015-9458-x
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