Please use this identifier to cite or link to this item: http://hdl.handle.net/1893/29985
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dc.contributor.authorRamkissoona, Nisha Ken_UK
dc.contributor.authorPearson, Victoria Ken_UK
dc.contributor.authorSchwenzer, Susanne Pen_UK
dc.contributor.authorSchröder, Christianen_UK
dc.contributor.authorKirnbauer, Thomasen_UK
dc.contributor.authorWood, Deborahen_UK
dc.contributor.authorSeidel, Robert G Wen_UK
dc.contributor.authorMiller, Michael Aen_UK
dc.contributor.authorOlsson-Francis, Karenen_UK
dc.date.accessioned2019-08-13T00:01:12Z-
dc.date.available2019-08-13T00:01:12Z-
dc.date.issued2019-08-10en_UK
dc.identifier.urihttp://hdl.handle.net/1893/29985-
dc.description.abstractExisting martian simulants are predominantly based on the chemistry of the average ‘global’ martian regolith as defined by data on chemical and mineralogical variability detected by orbiting spacecraft, surface rovers and landers. We have therefore developed new martian simulants based on the known composition of regolith from four different martian surface environments: an early basaltic terrain, a sulfur-rich regolith, a haematite-rich regolith and a contemporary Mars regolith. Simulants have been developed so that the Fe2+/Fe3+ ratios can be adjusted, if necessary, leading to the development of four standard simulants and four Fe-modified simulants. Characterisation of the simulants confirm that all but two (both sulfur-rich) are within 5 wt% of the martian chemistries that they were based on and, unlike previous simulants, they have Fe2+/Fe3+ ratios comparable to those found on Mars. Here we outline the design, production and characterisation of these new martian regolith simulants. These are to be used initially in experiments to study the potential habitability of martian environments in which Fe may be a key energy source.en_UK
dc.language.isoenen_UK
dc.publisherElsevieren_UK
dc.relationRamkissoona NK, Pearson VK, Schwenzer SP, Schröder C, Kirnbauer T, Wood D, Seidel RGW, Miller MA & Olsson-Francis K (2019) New simulants for martian regolith: controlling iron variability. Planetary and Space Science. https://doi.org/10.1016/j.pss.2019.104722en_UK
dc.rightsThis item has been embargoed for a period. During the embargo please use the Request a Copy feature at the foot of the Repository record to request a copy directly from the author. You can only request a copy if you wish to use this work for your own research or private study.en_UK
dc.subjectSimulanten_UK
dc.subjectMarsen_UK
dc.subjectRegolithen_UK
dc.subjectIronen_UK
dc.subjectHabitabilityen_UK
dc.subjectSimulationen_UK
dc.titleNew simulants for martian regolith: controlling iron variabilityen_UK
dc.typeJournal Articleen_UK
dc.rights.embargodate2020-08-11en_UK
dc.identifier.doi10.1016/j.pss.2019.104722en_UK
dc.citation.jtitlePlanetary and Space Scienceen_UK
dc.citation.issn0032-0633en_UK
dc.citation.publicationstatusPublisheden_UK
dc.citation.peerreviewedRefereeden_UK
dc.type.statusAM - Accepted Manuscripten_UK
dc.contributor.funderThe Leverhulme Trusten_UK
dc.author.emailchristian.schroeder@stir.ac.uken_UK
dc.citation.date10/08/2019en_UK
dc.contributor.affiliationThe Open Universityen_UK
dc.contributor.affiliationThe Open Universityen_UK
dc.contributor.affiliationThe Open Universityen_UK
dc.contributor.affiliationBiological and Environmental Sciencesen_UK
dc.contributor.affiliationTechnische Hochschule Georg Agricolaen_UK
dc.contributor.affiliationBiological and Environmental Sciencesen_UK
dc.contributor.affiliationThe Open Universityen_UK
dc.contributor.affiliationSouthwest Research Instituteen_UK
dc.contributor.affiliationThe Open Universityen_UK
dc.identifier.wtid1425943en_UK
dc.contributor.orcid0000-0002-7935-6039en_UK
dc.date.accepted2019-08-09en_UK
dc.description.refREF Compliant by Deposit in Stirling's Repositoryen_UK
dc.date.filedepositdate2019-08-12en_UK
Appears in Collections:Biological and Environmental Sciences Journal Articles

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