MR13A-2683
Volatile-refractory element reactions and breakdown of refractory oxides under conditions of a giant impact

Monday, 14 December 2015
Poster Hall (Moscone South)
Oliver D Tschauner, University of Nevada Las Vegas, Las Vegas, NV, United States and Chi Ma, California Institute of Technology, Pasadena, CA, United States
Abstract:
Whereas much or most of the highly volatile elements reside in atmosphere and oceans, understanding the global budget of these elements requires knowledge about their abundance in the Earth’s interior. One piece of this puzzle is the early history of the Earth where large impacts, notably giant impacts, provided conditions where both volatile and refractory elements were mixed on atomic scale in extremely hot dense fluids. Carbides and nitrides that have recently been found in mantle rock are possible remnants of such large scale dynamic pressure-temperature conditions. In particular carbides and nitrides of lithophile refractory elements like Zr, Hf, Nb, Ta may remain in the mantle for extended time and contribute to the mantle geochemical budget of these elements as well as that of C and N.

In a first step towards testing such a hypothesis, we conducted a series of shock experiments. Deflagration of C-N-O-H compounds was triggered by shockwaves. The resulting reaction wave front propagated into aggregates of refractory minerals like zircon, baddeleyite, rutile. This fluid-solid mix was subjected to shock compression to shock pressures of 20-50 GPa and temperatures in the range of 0.5-1.104 K by means of reverberating shock. Recovered sample material was analyzed by synchrotron X-ray diffraction and by EPMA.