To what extent does terrestrial life "Follow The Water"?
Terrestrial life is known to require liquid water, but not all terrestrial water is inhabited. Thus, liquid water is a necessary, but not sufficient, condition for life. To quantify the terrestrial limits on the habitability of water and help identify the factors that make some terrestrial water uni...
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Mary Ann Liebert
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ftanucanberra:oai:openresearch-repository.anu.edu.au:1885/8711 2024-01-14T10:07:36+01:00 To what extent does terrestrial life "Follow The Water"? Jones, Eriita Lineweaver, Charles 24 pages http://hdl.handle.net/1885/8711 https://doi.org/10.1089/ast.2009.0428 https://openresearch-repository.anu.edu.au/bitstream/1885/8711/4/JonesEriita_ToWhatExtent2010.pdf.jpg unknown Mary Ann Liebert 1531-1074 1557-8070 http://hdl.handle.net/1885/8711 doi:10.1089/ast.2009.0428 https://openresearch-repository.anu.edu.au/bitstream/1885/8711/4/JonesEriita_ToWhatExtent2010.pdf.jpg http://www.sherpa.ac.uk/romeo/issn/1531-1074/ " . author cannot archive pre-print (ie pre-refereeing) . Author can archive post-print (ie final draft post-refereeing) . [and] publisher's version/PDF . on own website, institution's intranet, or institutional repository. Authors may deposit in funding agency designated repository after 12 months. Set statement to accompany deposit (see policy). Publisher copyright and source must be acknowledged" - from SHERPA/RoMEO site (as at 2/11/11) Astrobiology 10.3 (2010): 349-361 biosphere limits of life extremophiles water Journal article ftanucanberra https://doi.org/10.1089/ast.2009.0428 2023-12-15T09:34:56Z Terrestrial life is known to require liquid water, but not all terrestrial water is inhabited. Thus, liquid water is a necessary, but not sufficient, condition for life. To quantify the terrestrial limits on the habitability of water and help identify the factors that make some terrestrial water uninhabited, we present empirical pressure-temperature (P-T) phase diagrams of water, Earth, and terrestrial life. Eighty-eight percent of the volume of Earth where liquid water exists is not known to host life. This potentially uninhabited terrestrial liquid water includes i) hot and deep regions of Earth where some combination of high temperature (T > 122˚C) and restrictions on pore space, nutrients, and energy is the limiting factor, and ii) cold and near surface regions of Earth, such as brine inclusions and thin films in ice and permafrost (depths less than ~1 km), where low temperatures (T < - 40˚C), low water activity (aw < 0.6), or both are the limiting factors. If the known limits of terrestrial life do not change significantly, these limits represent important constraints on our biosphere and, potentially, on others, since ~4 billion years of evolution have not allowed life to adapt to a large fraction of the volume of Earth where liquid water exists. Article in Journal/Newspaper Ice permafrost Australian National University: ANU Digital Collections Astrobiology 10 3 349 361 |
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Australian National University: ANU Digital Collections |
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ftanucanberra |
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unknown |
topic |
biosphere limits of life extremophiles water |
spellingShingle |
biosphere limits of life extremophiles water Jones, Eriita Lineweaver, Charles To what extent does terrestrial life "Follow The Water"? |
topic_facet |
biosphere limits of life extremophiles water |
description |
Terrestrial life is known to require liquid water, but not all terrestrial water is inhabited. Thus, liquid water is a necessary, but not sufficient, condition for life. To quantify the terrestrial limits on the habitability of water and help identify the factors that make some terrestrial water uninhabited, we present empirical pressure-temperature (P-T) phase diagrams of water, Earth, and terrestrial life. Eighty-eight percent of the volume of Earth where liquid water exists is not known to host life. This potentially uninhabited terrestrial liquid water includes i) hot and deep regions of Earth where some combination of high temperature (T > 122˚C) and restrictions on pore space, nutrients, and energy is the limiting factor, and ii) cold and near surface regions of Earth, such as brine inclusions and thin films in ice and permafrost (depths less than ~1 km), where low temperatures (T < - 40˚C), low water activity (aw < 0.6), or both are the limiting factors. If the known limits of terrestrial life do not change significantly, these limits represent important constraints on our biosphere and, potentially, on others, since ~4 billion years of evolution have not allowed life to adapt to a large fraction of the volume of Earth where liquid water exists. |
format |
Article in Journal/Newspaper |
author |
Jones, Eriita Lineweaver, Charles |
author_facet |
Jones, Eriita Lineweaver, Charles |
author_sort |
Jones, Eriita |
title |
To what extent does terrestrial life "Follow The Water"? |
title_short |
To what extent does terrestrial life "Follow The Water"? |
title_full |
To what extent does terrestrial life "Follow The Water"? |
title_fullStr |
To what extent does terrestrial life "Follow The Water"? |
title_full_unstemmed |
To what extent does terrestrial life "Follow The Water"? |
title_sort |
to what extent does terrestrial life "follow the water"? |
publisher |
Mary Ann Liebert |
url |
http://hdl.handle.net/1885/8711 https://doi.org/10.1089/ast.2009.0428 https://openresearch-repository.anu.edu.au/bitstream/1885/8711/4/JonesEriita_ToWhatExtent2010.pdf.jpg |
genre |
Ice permafrost |
genre_facet |
Ice permafrost |
op_source |
Astrobiology 10.3 (2010): 349-361 |
op_relation |
1531-1074 1557-8070 http://hdl.handle.net/1885/8711 doi:10.1089/ast.2009.0428 https://openresearch-repository.anu.edu.au/bitstream/1885/8711/4/JonesEriita_ToWhatExtent2010.pdf.jpg |
op_rights |
http://www.sherpa.ac.uk/romeo/issn/1531-1074/ " . author cannot archive pre-print (ie pre-refereeing) . Author can archive post-print (ie final draft post-refereeing) . [and] publisher's version/PDF . on own website, institution's intranet, or institutional repository. Authors may deposit in funding agency designated repository after 12 months. Set statement to accompany deposit (see policy). Publisher copyright and source must be acknowledged" - from SHERPA/RoMEO site (as at 2/11/11) |
op_doi |
https://doi.org/10.1089/ast.2009.0428 |
container_title |
Astrobiology |
container_volume |
10 |
container_issue |
3 |
container_start_page |
349 |
op_container_end_page |
361 |
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1788061984222085120 |