000103632 001__ 103632
000103632 005__ 20230824003325.0
000103632 0247_ $$2doi$$a10.7936/6rxs-103632
000103632 037__ $$aRDM
000103632 041__ $$aeng
000103632 245__ $$aMineral Products and Fluid Compositions From the Transformations of Iron(III) Minerals in Mars-Relevant Fluids
000103632 260__ $$bWashington University in St. Louis
000103632 269__ $$a2023-05-26
000103632 270__ $$malknight@wustl.edu$$pAbigail Knight
000103632 336__ $$aDataset
000103632 518__ $$d2019-09-01/2023-05-21$$oCollected
000103632 520__ $$aVera Rubin ridge (VRR), located in Gale crater, Mars, contains coarse-grained (>3-5 µm) gray hematite particles. VRR likely experienced multiple episodes of diagenesis in its past, some of which may have formed gray hematite from existing iron(III) minerals. The precursor mineralogy and diagenetic fluid conditions, however, are unknown. Experiments were performed on several iron(III) minerals (akaganeite, ferrihydrite, goethite, red hematite, jarosite, and schwertmannite) to simulate transformations in diagenetic fluid conditions. The solid transformation products were analyzed via powder X-ray diffraction, visible to near-infrared reflectance spectroscopy, and scanning electron microscopy. The compositions of the final fluids were determined via inductively-coupled plasma optical emission spectrometry. Final pH values of the fluid products were measured as well.
000103632 536__ $$oNational Aeronautics and Space Administration$$qhttps://ror.org/027ka1x80$$rROR$$c80NSSC19K1521$$aNASA Science Mission Directorate Future Investigators in NASA Earth and Space Science and Technology (FINESST)
000103632 536__ $$oNational Aeronautics and Space Administration$$qhttps://ror.org/027ka1x80$$rROR$$c80NSSC18K1292$$aNASA Exobiology program
000103632 536__ $$oWashington University in St. Louis$$qhttps://ror.org/01yc7t268$$rROR
000103632 540__ $$aCreative Commons Attribution (CC BY) 4.0 International$$uhttps://creativecommons.org/licenses/by/4.0/
000103632 650__ $$aPhysical sciences
000103632 650__ $$aEarth and related environmental sciences
000103632 6531_ $$aHematite
000103632 6531_ $$aJarosite
000103632 6531_ $$aVera Rubin ridge
000103632 6531_ $$aDiagenesis
000103632 6531_ $$aGale crater
000103632 6531_ $$aMars
000103632 655__ $$aImage
000103632 655__ $$aTabular
000103632 7001_ $$aKnight, Abigail$$1https://orcid.org/0000-0001-6832-8190$$uWashington University in St. Louis$$4https://ror.org/01yc7t268$$5ROR
000103632 7001_ $$aMitra, Kaushik$$1https://orcid.org/0000-0001-9673-1032$$uStony Brook University$$4https://ror.org/05qghxh33$$5ROR
000103632 7001_ $$aCatalano, Jeffrey G.$$1https://orcid.org/0000-0001-9311-977X$$uWashington University in St. Louis$$4https://ror.org/01yc7t268$$5ROR
000103632 720__ $$aWashU Institute of Materials Science and Engineering$$uWashington University in St. Louis$$4https://ror.org/01yc7t268$$5ROR$$eResearchGroup$$7Organizational
000103632 720__ $$aArvidson, Raymond$$uWashington University in St. Louis$$1https://orcid.org/0000-0002-2854-0362$$4https://ror.org/01yc7t268$$5ROR$$eDataCollector$$7Personal
000103632 720__ $$aCarpenter, Paul$$uWashington University in St. Louis$$1https://orcid.org/0000-0002-4639-3247$$4https://ror.org/01yc7t268$$5ROR$$eDataCollector$$7Personal
000103632 720__ $$aFlynn, Elaine$$uWashington University in St. Louis$$1https://orcid.org/0000-0002-1164-0148$$4https://ror.org/01yc7t268$$5ROR$$eDataCollector$$7Personal
000103632 8564_ $$97496fc5e-31db-4353-bfa3-28c1043c5e2d$$s201446676$$uhttps://data.library.wustl.edu/record/103632/files/Knight_Iron_Oxide_Transformation_Products.zip$$ePublic$$206df18290376f82c749751e75bf5f5bf$$03
000103632 8564_ $$yReadme file$$91f7873be-1153-4251-829e-66ad85db700a$$s28197$$uhttps://data.library.wustl.edu/record/103632/files/readme_doi1079366rxs103632_Knight.txt$$ePublic$$202c26ba7c09d1405cfd4ae08dfc0bb12$$03
000103632 909CO $$ooai:data.library.wustl.edu:103632$$pdataset
000103632 974__ $$aMars
000103632 980__ $$aWashU Researcher Data