Seventh International Conference on Mars 3156.pdf MARS LATITUDE, MARS OBLIQUITY, AND HYDRATION STATES OF Mg-SULFATES. D. T. Vani- man1, S. J. Chipera1, D. L Bish2, and R. C. Peterson3, 1Group EES-6, MS D462, Los Alamos National Laboratory, Los Alamos, NM 87545 (
[email protected];
[email protected]), 2Dept. of Geological Sciences, Indiana Univ., 1001 E. 10th St., Bloomington, IN 47405 (
[email protected]), 3Dept. of Geological Sciences and Geological Engi- neering, Queen’s Univ., Kingston, Ontario, K7L 3N6, Canada (
[email protected]). Introduction: Mg-sulfate minerals and synthetic phases exist in many hydration states, from anhydrous forms that are synthesized commercially to the com- mon retail product epsomite (MgSO4·7H2O) and the newly described synthetic 11-hydrate [1] and its natu- ral equivalent [see abstract by Peterson in this vol- ume]. Table 1 summarizes a variety of Mg-sulfate forms as described in [1] and [2]. Table 1: Forms of Mg-sulfate hydrates Formula Mineral name MgSO4 anhydrous none (reagent) MgSO4·1H2O kieserite MgSO4·1H2O type 2 none (reagent) MgSO4·2H2O sanderite MgSO4·2.4H2O none MgSO ·4H O starkeyite 4 2 MgSO4·5H2O pentahydrite The 11-hydrate form of Mg-sulfate (Figure 1) may MgSO4·6H2O hexahydrite be a stable phase on Mars under current higher-latitude MgSO4·7H2O epsomite conditions where water ice is present to maintain high MgSO4·11H2O pending approval by IMA* relative humidity, albeit at very low pH2O. At lower MgSO4·nH2O amorphous (n variable) latitudes, where daytime relative humidity is very low, *International Mineralogical Association the more likely form of Mg-sulfate hydrate may be either kieserite or an amorphous form with water con- It is conceivable that any of these Mg-sulfate tent dependent at least in part on temperature [5,6].