Cooling History of Almahata Sitta Ureilite as Inferred from Transmission Electron Microscopy of Iron MetalAlmahata Sitta (AS) is a polymict breccia mainly composed of various ureilite lithologies with lesser chondritic lithologies [1]. In the ureilite lithologies, Fe metal is a common accessory phase present either as large grain boundary grains or small particles formed by reduction of olivine and pyroxene. In our earlier studies on grain boundary metals in one of AS fragments (#44) we found unique features never seen in other ureilites [2,3]. In order to further characterize these metal grains, we performed a detailed TEM study on a FIB section prepared from one of AS #44 grain boundary metals and here discuss its thermal history.
Document ID
20140000761
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Mikouchi, T. (Tokyo Univ. Japan)
Aoyagi, Y. (Tokyo Univ. Japan)
Goodrich, C. A. (Planetary Science Inst. Tucson, AZ, United States)
Yubuta, K. (Tohoku Univ. Sendai, Japan)
Sugiyama, K. (Tohoku Univ. Sendai, Japan)
Zolensky, M. E. (NASA Johnson Space Center Houston, TX, United States)
Goldstein, J. I. (Massachusetts Univ. Amherst, MA, United States)