Iron Meteorites
      Iron meteorites are composed largely of nickel-iron metal, and most
      contain only minor accessory minerals. These accessory minerals often
      occur in rounded nodules that consist of the iron-sulfide troilite or
      graphite, often surrounded by the iron-phosphide schreibersite and the
      iron-carbide cohenite. Despite the fact that some iron meteorites contain
      silicate inclusions, most have fundamentally the same superficial
      appearance.
       Presently, iron meteorites are classified under two established systems.
      Just a few decades ago, iron meteorites were exclusively classified
      according to the macroscopic structures revealed when their polished
      surface was etched with nitric acid. Depending on these structures, they
      were separated into three classes: octahedrites, hexahedrites, and
      ataxites.  
      IIIAB Group
      With about 233 members, group IIIAB is the best-represented class of
      iron meteorites in our collections. Compared to the members of the IIIA
      subgroup, which have mostly coarse octahedrite textures, the IIIB irons
      usually display medium textures. Still, the members of both subgroups form
      a continuous sequence in structural and elemental compositions that
      suggests a common origin, probably representing different regions of an
      asteroid's core. Group IIIAB contains several prominent members
      representing some of the largest irons ever found. Just to name a few,
      there are the giants of Cape York, Chupaderos, Morito, and Willamette -
      have a look at our charts. Some
      IIIAB members contain large nodules of troilite and graphite, but silicate
      inclusions are rare. Despite this fact, recent research suggests a close
      relationship exists between the IIIAB irons and the silicate-rich main
      group pallasites, some of the most attractive stony-iron meteorites
      known. Both groups probably formed on the same parent body, a
      differentiated asteroid that was disrupted by a single impact event. The
      IIIAB iron meteorites represent fragments of the core, while the
      main-group pallasites are samples of the core/mantle boundary of this
      common parent body. 
        
      
        
        
          
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              Henbury 
             
            IIIAB     
            Year found: 1931 
            Country: Australia 
            TKW : 2 MT 
              
        
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            	Henbury-00
               Complete oriented henbury, really pretty ! 
              SOLD 
              Price
              on request	  | 
         
        
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             Henbury-01 
            Complete slice showing nice structure ! 
            176 gr 
            875 $ 
             
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