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An Extensive Phase Space for the Potential Martian Biosphere

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dc.contributor.authorJones, Eriita
dc.contributor.authorClarke, Jonathon
dc.contributor.authorLineweaver, Charles
dc.date.accessioned2015-12-10T22:15:14Z
dc.date.issued2011
dc.date.updated2016-02-24T09:54:23Z
dc.description.abstractWe present a comprehensive model of martian pressure-temperature (P-T) phase space and compare it with that of Earth. Martian P-T conditions compatible with liquid water extend to a depth of ∼310km. We use our phase space model of Mars and of terrestria
dc.identifier.issn1531-1074
dc.identifier.urihttp://hdl.handle.net/1885/50552
dc.publisherMary Ann Liebert Inc.
dc.sourceAstrobiology
dc.subjectKeywords: water; article; astronomy; pressure; soil; temperature; theoretical model; Mars; Models, Theoretical; Pressure; Soil; Temperature; Water Biosphere; Extremophiles; Limits of life; Mars; Water
dc.titleAn Extensive Phase Space for the Potential Martian Biosphere
dc.typeJournal article
local.bibliographicCitation.issue10
local.bibliographicCitation.lastpage1033
local.bibliographicCitation.startpage1017
local.contributor.affiliationJones, Eriita, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationLineweaver, Charles, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationClarke, Jonathon, Mars Society Australia Inc
local.contributor.authoruidJones, Eriita, u2522213
local.contributor.authoruidLineweaver, Charles, u4186476
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.identifier.absfor020101 - Astrobiology
local.identifier.absfor020108 - Planetary Science (excl. Extraterrestrial Geology)
local.identifier.absseo970104 - Expanding Knowledge in the Earth Sciences
local.identifier.ariespublicationu3356449xPUB206
local.identifier.citationvolume11
local.identifier.doi10.1089/ast.2011.0660
local.identifier.scopusID2-s2.0-84555188137
local.identifier.thomsonID000298345600006
local.type.statusPublished Version

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