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MIB 03002

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Journal Article
Published: 01 November 2006
European Journal of Mineralogy (2006) 18 (6): 727–738.
...Massimo D’Orazio; Luigi Folco; Kees C. Welten; Marc W. Caffee; Natale Perchiazzi; Pierre Rochette Abstract The Miller Butte (MIB) 03002 iron meteorite was found during the XIX (2003–2004) Antarctic campaign of the Italian Programma Nazionale delle Ricerche in Antartide (PNRA) in northern Victoria...
FIGURES | View All (10)
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<span class="search-highlight">MIB</span> <span class="search-highlight">03002</span> iron meteorite as found. Arrows point to the grooves arranged in ...
Published: 01 November 2006
Fig. 2. MIB 03002 iron meteorite as found. Arrows point to the grooves arranged in Widmanstätten pattern on some points of the surface.
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Etched cut surface on the main mass of <span class="search-highlight">MIB</span> <span class="search-highlight">03002</span>. The kamacite lamellae of ...
Published: 01 November 2006
Fig. 3. Etched cut surface on the main mass of MIB 03002. The kamacite lamellae of the Widmanstätten pattern are oriented in three different directions at ~ 60°. Inset: detail of the etched cut surface on the main mass of MIB 03002, showing a 8.5 mm trace of a shear-displacement plane through
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Estimated pre-entry radius for Miller Butte (<span class="search-highlight">MIB</span>) <span class="search-highlight">03002</span> compared to those o...
Published: 01 November 2006
Fig. 10. Estimated pre-entry radius for Miller Butte (MIB) 03002 compared to those of other 14 iron meteorites. Radii for the latter meteorites were calculated, following the LCS model of Masarik & Reedy (1994) , on the basis of the pre-entry 10 Be and 36 Cl radionuclide activities given
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(a) Sketch map of northern Victoria Land Antarctica, showing the location o...
Published: 01 November 2006
Fig. 1. (a) Sketch map of northern Victoria Land Antarctica, showing the location of Miller Butte and its drainage area extending eastward up to Talos Dome. (b) Satellite image map of the Miller Butte area showing ice flow (arrows) and the site of MIB 03002 finding. (c) Aerial view of the Miller
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Plots of Ga (a), Ge (b) and Ir (c) vs. Ni showing the fields for the 13 iro...
Published: 01 November 2006
Fig. 6. Plots of Ga (a), Ge (b) and Ir (c) vs. Ni showing the fields for the 13 iron meteorite groups. Axes are in logarthmic scale. MIB 03002 falls within the field of IID irons.
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Comparison of measured concentrations of  10 Be (a) and  36 Cl (b) in <span class="search-highlight">MIB</span> 0...
Published: 01 November 2006
Fig. 8. Comparison of measured concentrations of 10 Be (a) and 36 Cl (b) in MIB 03002, corrected for radioactive decay since the time of fall, with calculated production rates (in atoms min −1 kg −1 ) as a function of size and depth ( Welten et al. , 2001a and b ).
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Plots of As (a) and Re (b) vs. Ir for the iron meteorites of group IID. The...
Published: 01 November 2006
Fig. 7. Plots of As (a) and Re (b) vs. Ir for the iron meteorites of group IID. The trends delineated by the data points are consistent with a prevailing fractional crystallization process. Grey arrows point towards the most evolved members. MIB 03002 plots approximately halfway the trend. Data
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Reflected plane polarized light photomicrographies (a, b) and secondary ele...
Published: 01 November 2006
Fig. 4. Reflected plane polarized light photomicrographies (a, b) and secondary electrons SEM images (c, d, d, f) of MIB 03002. (a)Kamacite lamella hosting a schreibersite crystal along its central portion. The recrystallized kamacite grains close to the schreibersite are larger, better