<HashMap><database>biostudies-literature</database><scores/><additional><submitter>Wildner M</submitter><funding>Austrian Science Fund FWF</funding><pagination>194-203</pagination><full_dataset_link>https://www.ebi.ac.uk/biostudies/studies/S-EPMC8895014</full_dataset_link><repository>biostudies-literature</repository><omics_type>Unknown</omics_type><volume>9(Pt 2)</volume><pubmed_abstract>Monohydrate sulfate kieserites (&lt;i>M&lt;/i> &lt;sup>2+&lt;/sup>SO&lt;sub>4&lt;/sub>·H&lt;sub>2&lt;/sub>O) and their solid solutions are essential constituents on the surface of Mars and most likely also on Galilean icy moons in our solar system. Phase stabilities of end-member representatives (&lt;i>M&lt;/i> &lt;sup>2+&lt;/sup> = Mg, Fe, Co, Ni) have been examined crystallographically using single-crystal X-ray diffraction at 1 bar and temperatures down to 15 K, by means of applying open He cryojet techniques at in-house laboratory instrumentation. All four representative phases show a comparable, highly anisotropic thermal expansion behavior with a remarkable negative thermal expansion along the monoclinic &lt;i>b&lt;/i> axis and a pronounced anisotropic expansion perpendicular to it. The lattice changes down to 15 K correspon</pubmed_abstract><journal>IUCrJ</journal><pubmed_title>Crystallography relevant to Mars and Galilean icy moons: crystal behavior of kieserite-type monohydrate sulfates at extraterrestrial conditions down to 15 K.</pubmed_title><pmcid>PMC8895014</pmcid><funding_grant_id>P 29149-N29</funding_grant_id><pubmed_authors>Miletich R</pubmed_authors><pubmed_authors>Zakharov BA</pubmed_authors><pubmed_authors>Bogdanov NE</pubmed_authors><pubmed_authors>Boldyreva EV</pubmed_authors><pubmed_authors>Talla D</pubmed_authors><pubmed_authors>Wildner M</pubmed_authors></additional><is_claimable>false</is_claimable><name>Crystallography relevant to Mars and Galilean icy moons: crystal behavior of kieserite-type monohydrate sulfates at extraterrestrial conditions down to 15 K.</name><description>Monohydrate sulfate kieserites (&lt;i>M&lt;/i> &lt;sup>2+&lt;/sup>SO&lt;sub>4&lt;/sub>·H&lt;sub>2&lt;/sub>O) and their solid solutions are essential constituents on the surface of Mars and most likely also on Galilean icy moons in our solar system. Phase stabilities of end-member representatives (&lt;i>M&lt;/i> &lt;sup>2+&lt;/sup> = Mg, Fe, Co, Ni) have been examined crystallographically using single-crystal X-ray diffraction at 1 bar and temperatures down to 15 K, by means of applying open He cryojet techniques at in-house laboratory instrumentation. All four representative phases show a comparable, highly anisotropic thermal expansion behavior with a remarkable negative thermal expansion along the monoclinic &lt;i>b&lt;/i> axis and a pronounced anisotropic expansion perpendicular to it. The lattice changes down to 15 K correspon</description><dates><release>2022-01-01T00:00:00Z</release><publication>2022 Mar</publication><modification>2025-04-04T07:48:07.712Z</modification><creation>2025-04-04T07:48:07.712Z</creation></dates><accession>S-EPMC8895014</accession><cross_references><pubmed>35371501</pubmed><doi>10.1107/S2052252521012720</doi></cross_references></HashMap>