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1 Dipartimento di Scienze della Terra, Università di Pisa, 56126 Pisa, Italy
2 Istituto di Geoscienze e Georisorse, Sezione di Pisa, C.N.R., 56124 Pisa, Italy
3 Museo Nazionale dellAntartide, 53100 Siena, Italy
4 Space Sciences Laboratory, University of California, Berkeley, CA 947207450, USA
5 Department of Physics, Purdue University, West Lafayette, IN 47907, USA.
4 CEREGE, CNRS Université dAix-Marseille III, PB80 13545, Aix en Provence, Cdx 4, France
* Corresponding author, e-mail: dorazio{at}dst.unipi.it
The Miller Butte (MIB) 03002 iron meteorite was found during the XIX (20032004) Antarctic campaign of the Italian Programma Nazionale delle Ricerche in Antartide (PNRA) in northern Victoria Land (Antarctica). MIB 03002 is classified as a medium octahedrite belonging to the rare IID chemical group, and it is the first IID iron among the 30,000 specimens so far returned from Antarctica. The bulk chemistry of this meteorite indicates that it represents an intermediate member of the differentiation series of IID irons. Polygonal kamacite, shear planes in the Widmanstätten structure and relics of cross-hatched
-structure indicate that MIB 03002 experienced important shock metamorphism (T
700 °C and P
13 GPa) and post-shock annealing, after primary cooling. With a terrestrial age of ~ 610 ka, MIB 03002 is the oldest meteorite fall in northern Victoria Land so far, and the oldest Antarctic iron found on blue ice. Possible relationships between the old terrestrial age of MIB 03002 and the regional glacial dynamics of the East Antarctic Ice Sheet in northern Victoria Land are also discussed.
Key-words: iron meteorites, terrestrial age, cosmogenic nuclides, Antarctica, northern Victoria Land, Miller Butte.
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