Show simple item record

dc.contributor.authorCullen, M. D.
dc.contributor.authorPhillips-Lander, C. M.
dc.contributor.authorElwood Madden, A. S.
dc.contributor.authorElwood Madden, M. E.
dc.date.accessioned2021-11-22T19:04:07Z
dc.date.available2021-11-22T19:04:07Z
dc.date.issued2021-08-24
dc.identifier.citationCullen, M. Elwood Madden A.S., Phillips-Lander, C.M., and Elwood Madden, M.E. (2021) Siderite Dissolution in Mars-Analog Brines: Kinetics and Reaction Products. Planetary Science Journal, 2(5), p. 169 https://doi.org/10.3847/PSJ/ac13a3en_US
dc.identifier.urihttps://hdl.handle.net/11244/331271
dc.description.abstractThis study examines siderite (FeCO3) reactivity in MgCl2 and MgSO4 brines with varying salt concentrations (0.01M, 1M, and 3M) at both acidic (pH ∼ 2 and pH ≤ 2) and near-neutral (pH ∼ 7) conditions. We measured aqueous Fe concentrations through time to determine dissolution rates and characterized the solid reaction products with scanning electron microscopy, electron dispersive X-ray spectroscopy, and Raman spectroscopy. Iron-based siderite dissolution rates at pH 2 were equivalent in the 0.01M and 1M MgSO4 brines and slower in 3M MgSO4; rates in the MgCl2 brines slow systematically with increasing brine concentration for equivalent initial pH values. Fe-based dissolution rates could not be determined in the neutral pH experiments due to precipitation of iron (hydr)oxide phases. After 1 day in acidic brines, abundant etch pits were observed; however, in the neutral experiments, siderite was identified with Raman spectroscopy even after 1 yr of dissolution along with a range of iron (hydr)oxide phases. Scanning electron microscopy imaging of the neutral experiment products found Mg-sulfate brines produced a chaotic surface texture. Therefore, micron-scale textural observations could be used to discriminate between alteration in chloride and sulfate brines. Initial iron release rates were similar in dilute brines, but decreased by less than an order of magnitude in the two highest-concentration pH 2 brine experiments; therefore, siderite-bearing assemblages exposed to acidic fluids, regardless of salinity, would likely dissolve completely over geologically short periods of time, thus erasing siderite and likely other carbonate minerals from the geologic record.en_US
dc.description.sponsorshipFunding was provided by NASA grant #NNX13AG75G and the School of Geosciences at the University of Oklahoma.en_US
dc.languageen_USen_US
dc.rightsAttribution 4.0 International*
dc.rights.urihttps://creativecommons.org/licenses/by/4.0/*
dc.subjectMarsen_US
dc.titleSiderite Dissolution in Mars-analog Brines: Kinetics and Reaction Productsen_US
dc.typeArticleen_US
dc.description.peerreviewYesen_US
dc.identifier.doi10.3847/PSJ/ac13a3en_US
ou.groupMewbourne College of Earth and Energy::School of Geosciencesen_US


Files in this item

Thumbnail
Thumbnail

This item appears in the following Collection(s)

Show simple item record


Attribution 4.0 International
Except where otherwise noted, this item's license is described as Attribution 4.0 International