Paper No. 4
Presentation Time: 1:30 PM-5:30 PM
FE-MG CARBONATE SOLID SOLUTION EXPERIMENTS LEAD TO FE-MG OXIDE SOLID SOLUTION EXPERIMENTS
KOZIOL, Andrea M., Geology, Univ of Dayton, 300 College Park, Dayton, OH 45469-2364, koziol@notes.udayton.edu
The mixing properties of siderite (sid;FeCO
3) - magnesite (magn; MgCO
3) solid solutions were to be measured via displaced equilibrium experiments performed in a piston-cylinder apparatus. The univariant reaction sid + hematite (hem; Fe
2O
3)=magnetite (mt; Fe
3O
4) + CO
2 is displaced to higher temperatures (at constant pressure) by the increasing mole % of magn in carbonate. Crystalline materials with AgC
2O
4 as CO
2 source, buffered at hem/mt in a double capsule, were held at 640°C - 660°C and 11 kbar for 3-5 days. All hem disappeared and mt apparently grew as shown by XRD analysis. However, I suggest magnesioferrite (mfer; MgFe
2O
4) formed from the hem and carbonate. Further research shows that mfer or mfer-mt solid solutions are stable at an oxygen fugacity (f
O2) of hem/mt or higher (at 1000°C). At lower f
O2 (or more Mg-rich compositions) a mfer-mt solid solution coexists with magnesiowustite (mwu; (Fe,Mg)O) (Zalazinskii et al. 1975, Russ. Jour. Phys. Chem. 49, 914-915). These phase relationships are under investigation now in this lab. Fe-Mg carbonate experiments as designed are not possible.
Applications: Controversy surrounds Martian meteorite ALH84001, especially the interpretation of carbonate globules and associated mt grains. The nanometer-sized, chemically pure mt grains have been cited as evidence for former life on Mars (McKay et al. 1996, Science 273, 924-930). However, they may have formed from Fe,Mg carbonate by increase in temperature or increase in environmental fO2 (Koziol 2003, XXXIV LPSC, Abst. #1128). If mt formed from sid-magn, this suggests a low fO2 (near mt/wustite) at formation. At higher fO2 mfer or mfer-mt solid solutions are stable. In a more general application, more study of Fe,Mg oxide stability (i.e. mwu) at high pressure and various temperatures and fO2 could shed light on phase relations in the mantles of Earth and Mars.
This research supported by NSF grant # EAR-9805873 and NASA grants # NAG5-8199 & NAG5-9808.