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IID meteorites

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Journal Article
Published: 01 November 2006
European Journal of Mineralogy (2006) 18 (6): 727–738.
... 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...
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Plots of As (a) and Re (b) vs. Ir for the iron <span class="search-highlight">meteorites</span> of group <span class="search-highlight">IID</span>. 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
Journal Article
Published: 01 August 2003
Mineralogical Magazine (2003) 67 (4): 783–792.
...R. Skála; M. Drábek Abstract The original description of nickelphosphide from the Butler meteorite [(Ni 1.83 Fe 1.21 ) ∑3.04 P 0.96 to (Ni 1.71 Fe 1.28 Co 0.01 ) ∑3.00 P 1.00 ] lacks detailed and accurate powder data – with only 11 observed reflections down to 1.37 Å. Consequently, no crystal...
FIGURES
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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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Schematic Ga vs. Ni and Ge vs. Ni log-log diagrams for iron <span class="search-highlight">meteorite</span> group...
Published: 01 January 2008
Figure 3. Schematic Ga vs. Ni and Ge vs. Ni log-log diagrams for iron meteorite groups showing the chemical classification of irons. Data sources are listed in the text and Table 3 . Older data were taken from Appendix IID of Wasson (1974) .
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Au concentration (ppm) of some representative <span class="search-highlight">meteorites</span> in different meteo...
Published: 13 February 2017
& Humayun ( 2009 ) **Jones ( 1968 ) Au concentration (ppm) 1.5 4.45 1.21 3.58 2.77 5.48 1.5 Iron meteorites IAB range of six meteorites analysed IIAB range of six meteorites analysed IID range of six meteorites analysed IIIAB range of nine meteorites analysed IIICD range of nine
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187 Re&#x2F; 188 Os versus  187 Os&#x2F; 188 Os diagrams for (a) IA, <span class="search-highlight">IID</span>, IB, IIIC, I...
Published: 01 January 2016
Figure 15 187 Re/ 188 Os versus 187 Os/ 188 Os diagrams for (a) IA, IID, IB, IIIC, IAB, IIIAB, (b) IVB, (c) IVA, (d) IIAB and (e) IIIAB iron meteorites and 190 Pt/ 188 Os versus 186 Os/ 188 Os diagram for (f) IIAB and IIIAB iron meteorites. Data and iso-/error-chrons are from Shen et al
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Correlation of  182 W/ 184 W with the  192 Pt excess induced by reactions o...
Published: 01 April 2023
Figure 3.22 Correlation of 182 W/ 184 W with the 192 Pt excess induced by reactions of cosmogenic thermal and epithermal neutrons on Pt and Ir isotopes for the two IID iron meteorites Rodeo and Carbo, which have nearly identical Ir/Pt ratios. The correlation defined by the Carbo data (which
Journal Article
Published: 01 April 2016
Geochemical Perspectives (2016) 5 (1): 21–35.
...) mantle of the body. The IID group does not fit the correlation ( Fig. 3.3 ). Kruijer et al . (2014a) called on the sequential core formation model of Wasson and Huber (2006) to explain the offset from the trend. Wasson and Huber (2006) suggested that, although relatively S-poor, the meteorites...
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Journal Article
Published: 01 September 2006
European Journal of Mineralogy (2006) 18 (5): 666.
... , P. R ochette . – Miller Butte 03002: a new rare iron meteorite (IID) from Antarctica. R. H einemann , H. K roll , A. K irfel , B. B arbier . – Order and anti-order in olivine. I. Structural response to temperature. H. K roll , A. K rifel , R. H einemann . – Order and anti-order in olivine...
Journal Article
Published: 01 June 2011
Russ. Geol. Geophys. (2011) 52 (6): 620–630.
...) of the chemical group IID ( Sobotovich and Semenenko, 1984 ). The general chemical composition of the Cheder meteorite is close to pallas iron ( D’yakonova et al., 1979 ) ( Table 1 ). Fig. 3. Width distribution of kamacite bars in the Cheder meteorite. The groundmass of the meteorite consists...
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Journal Article
Published: 01 January 2008
Reviews in Mineralogy and Geochemistry (2008) 68 (1): 571–590.
...Figure 3. Schematic Ga vs. Ni and Ge vs. Ni log-log diagrams for iron meteorite groups showing the chemical classification of irons. Data sources are listed in the text and Table 3 . Older data were taken from Appendix IID of Wasson (1974) . ...
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Journal Article
Journal: Geosphere
Published: 01 April 2008
Geosphere (2008) 4 (2): 445–458.
..., is defined by the Taghanic onlap, which is a major long-term episode of stepped eustatic sea-level rise that reached a maximum in the late Frasnian. This onlap was terminated by rapid eustatic sea-level fall within T-R cycle IId, during the end-Frasnian linguiformis Zone ( Johnson et al., 1985 ; Sandberg...
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Journal Article
Published: 01 January 2016
Reviews in Mineralogy and Geochemistry (2016) 81 (1): 107–160.
... “magmatic” iron meteorite group (e.g., IIAB, IID, IIIAB, IVA, and IVB) formed as part of a crystal-liquid fractionation sequence of genetically identical materials (e.g., Pernicka and Wasson 1987 ), irons of a given group should be expected to be characterized by identical anomalies. A third question...
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Journal Article
Published: 13 February 2017
Geological Magazine (2018) 155 (6): 1205–1229.
... & Humayun ( 2009 ) **Jones ( 1968 ) Au concentration (ppm) 1.5 4.45 1.21 3.58 2.77 5.48 1.5 Iron meteorites IAB range of six meteorites analysed IIAB range of six meteorites analysed IID range of six meteorites analysed IIIAB range of nine meteorites analysed IIICD range of nine...
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Journal Article
Published: 01 April 2023
Geochemical Perspectives (2023) 12 (1): 50–118.
...Figure 3.22 Correlation of 182 W/ 184 W with the 192 Pt excess induced by reactions of cosmogenic thermal and epithermal neutrons on Pt and Ir isotopes for the two IID iron meteorites Rodeo and Carbo, which have nearly identical Ir/Pt ratios. The correlation defined by the Carbo data (which...
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Journal Article
Journal: Economic Geology
Published: 01 March 2021
Economic Geology (2021) 116 (2): 471–500.
...-chalcopyrite-pyrite vein within tonalite porphyry. (D) Stage IIc quartz-chlorite-chalcopyrite vein and later disseminated molybdenite hosted by diorite porphyry. (E) Stage IId regular quartz-chalcopyrite-bornite ± pyrite vein overprinted by later 6-mm-wide quartz-chlorite halos. (F) Stage IId quartz-bornite...
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Journal Article
Published: 01 January 2016
Reviews in Mineralogy and Geochemistry (2016) 81 (1): 161–238.
...Figure 15 187 Re/ 188 Os versus 187 Os/ 188 Os diagrams for (a) IA, IID, IB, IIIC, IAB, IIIAB, (b) IVB, (c) IVA, (d) IIAB and (e) IIIAB iron meteorites and 190 Pt/ 188 Os versus 186 Os/ 188 Os diagram for (f) IIAB and IIIAB iron meteorites. Data and iso-/error-chrons are from Shen et al...
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Journal Article
Published: 01 November 1996
Jour. Geol. Soc. India (1996) 48 (5): 497–506.
... of 1678 ± 44 Ma Z'2 I-a CI) --to II) r--CI) (0 LlNGTSE GNEISS ~aE : une! lIn : 0'T2255! 0'010.8 IIS\IID: 17'~ '0 ~O 30 .0 50 eo TO 87Rb j86Sr Fig.2. Rb-Sr isochron plate for Lingtse Gneiss. with an initial Sr ratio of 0.722558 ± 0.010486 (MSWD=17.3). Whole rock Pb isotopic compositions (Table II...
Journal Article
Published: 01 May 2021
American Mineralogist (2021) 106 (5): 730–761.
... and Takeda 1985 ; Mittlefehldt et al. 1998 ). Cristobalite (SiO 2 ) . DA cristobalite is a minor phase in several eucrites, where it occurs in association with other silica polymorphs ( Aoudjehane and Jambon 2007 ), and as an accessory mineral in the troilite nodules of the Carbo (IID) iron meteorite...
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