46th Lunar and Planetary Science Conference (2015) 1825.pdf FORMATION OF JAROSITE MINERALS IN THE PRESENCE OF SEED MATERIAL H. E. A. Brand1,2 N. V. Y. Scarlett2 and I. E. Grey2, 1Australian Synchrotron, 800 Blackburn Rd., Clayton South, VIC 3168, Australia.
[email protected] 2CSIRO Mineral Resources, Box 312, Clayton, VIC 3187, Australia. Introduction: There has been a resurgence in interest Experimental method: Jarosite forms readily by co- in jarosite, (K,Na)Fe3(SO4)2(OH)6, and related precitation on gentle warming of an appropriate minerals since their detection on Mars by the MER solution. 2.25 g of Fe2(SO4)3.xH2O and 0.70 g of rover Opportunity [1]. In this context, the presence of K2SO4 were dissolved in 10 mls of deionized H2O. jarosite has been recognised as a likely indicator of Seed materials were diamond, hematite and goethite. water at the surface of Mars in the past and it is hoped Hematite and goethite are commonly found in that study of their formation mechanisms will provide association with natural jarosite deposits. The inclusion insight into the environmental history of Mars [2]. of diamond provides a baseline for the effect of an inert Jarosites are also of great importance to a range of seed material. These materials were added to the mineral processing and research applications. For jarosite starting-solutions to give 5 wt% seed. An example: they are used in the removal of iron species additional solution was prepared with no seed material from smelting processes; they form detrimentally in to provide a comparison set of data.