<HashMap><database>biostudies-literature</database><scores/><additional><submitter>Sklute EC</submitter><funding>NASA</funding><pagination>285-295</pagination><full_dataset_link>https://www.ebi.ac.uk/biostudies/studies/S-EPMC5901898</full_dataset_link><repository>biostudies-literature</repository><omics_type>Unknown</omics_type><volume>302</volume><pubmed_abstract>Salts with high hydration states have the potential to maintain high levels of relative humidity (RH) in the near subsurface of Mars, even at moderate temperatures. These conditions could promote deliquescence of lower hydrates of ferric sulfate, chlorides, and other salts. Previous work on deliquesced ferric sulfates has shown that when these materials undergo rapid dehydration, such as that which would occur upon exposure to present day Martian surface conditions, an amorphous phase forms. However, the fate of deliquesced halides or mixed ferric sulfate-bearing brines are presently unknown. Here we present results of rapid dehydration experiments on Ca-, Na-, Mg- and Fe-chloride brines and multi-component (Fe&lt;sub>2&lt;/sub> (SO&lt;sub>4&lt;/sub>)&lt;sub>3&lt;/sub> ± Ca, Na, Mg, Fe, Cl, HCO&lt;sub>3&lt;/sub>)</pubmed_abstract><journal>Icarus</journal><pubmed_title>Amorphous salts formed from rapid dehydration of multicomponent chloride and ferric sulfate brines: Implications for Mars.</pubmed_title><pmcid>PMC5901898</pmcid><funding_grant_id>NNX12AO45G</funding_grant_id><pubmed_authors>Rogers AD</pubmed_authors><pubmed_authors>Gregerson JC</pubmed_authors><pubmed_authors>Reeder RJ</pubmed_authors><pubmed_authors>Sklute EC</pubmed_authors><pubmed_authors>Jensen HB</pubmed_authors><pubmed_authors>Dyar MD</pubmed_authors></additional><is_claimable>false</is_claimable><name>Amorphous salts formed from rapid dehydration of multicomponent chloride and ferric sulfate brines: Implications for Mars.</name><description>Salts with high hydration states have the potential to maintain high levels of relative humidity (RH) in the near subsurface of Mars, even at moderate temperatures. These conditions could promote deliquescence of lower hydrates of ferric sulfate, chlorides, and other salts. Previous work on deliquesced ferric sulfates has shown that when these materials undergo rapid dehydration, such as that which would occur upon exposure to present day Martian surface conditions, an amorphous phase forms. However, the fate of deliquesced halides or mixed ferric sulfate-bearing brines are presently unknown. Here we present results of rapid dehydration experiments on Ca-, Na-, Mg- and Fe-chloride brines and multi-component (Fe&lt;sub>2&lt;/sub> (SO&lt;sub>4&lt;/sub>)&lt;sub>3&lt;/sub> ± Ca, Na, Mg, Fe, Cl, HCO&lt;sub>3&lt;/sub>)</description><dates><release>2018-01-01T00:00:00Z</release><publication>2018 Mar</publication><modification>2025-04-25T20:43:11.668Z</modification><creation>2019-03-26T23:29:36Z</creation></dates><accession>S-EPMC5901898</accession><cross_references><pubmed>29670302</pubmed><doi>10.1016/j.icarus.2017.11.018</doi></cross_references></HashMap>