Angrites
      The achondrites of this group are named for their type specimen, Angra
      dos Reis, a meteorite that fell in Rio de Janeiro, Brazil, in early 1869.
      Angra dos Reis is a unique igneous rock that is largely composed of the
      rare pyroxene fassaite, an aluminium-titanium diopside. During the last
      two decades, a handful of similar fassaite-rich meteorites have been
      recovered, leading to the establishment of the angrite group, presently
      comprising six members. 
      The angrites are primarily composed of varying amounts of fassaitic
      pyroxene, anorthitic plagioclase, minor olivine, kirschsteinite, along
      with other accessory minerals and phases. They are basaltic rocks with
      cumulate textures, often containing porous areas and abundant round
      vesicles with diameters up to 2.5 cm. These vesicles have been interpreted
      as remnants of gas-bubbles that formed prior to the crystallization of the
      rock. However, current research suggests that the vesicles originally were
      solid spheres that have been exsolved in subsequent stages of
      rock-formation. Both theories are consistent with a magmatic origin of the
      angrites, making them the most ancient igneous rocks known. They show
      crystallization ages of ~ 4.55 billion years, which suggests their
      formation occurred in the early days of the unfolding solar system. The
      angrites are thought to have formed on one of the earliest differentiated
      asteroids from the igneous processing of CAI-rich chondritic matter,
      similar to carbonaceous chondrites of the CI or CM group. 
      By comparing the reflectance spectra of the angrites to that of several
      main belt asteroids, two analogs were identified - 289 Nenetta, and 3819
      Robinson. Further research will determine whether one of these asteroids
      actually represents the angrite parent body. Only three angrites are
      currently available to the private collector; these are Sahara 99555, a
      single stone that was found in the Sahara desert in 1999,  D'Orbigny,
      an Argentinian find from 1979 that wasn't recognized as a meteorite until
      1998 and NWA 1670 with a total weight of only 30gr....  
        
       
       
        
        
          
            | 
            Sahara 99 555
             Angrite 
            Found in 1999, Sahara  
            2710 gr 
              
             | 
           
        
        
            
              
             | 
             | 
             | 
            	 | 
            	Sahara
              99555-01
               0.500 gr 
              Nice fragment for this rare type ! 
              SOLD	  | 
         
        
            | 
             | 
             | 
             | 
            	 | 
            	 | 
         
        
            | 
             Sahara 99555-02 
            0.354 gr 
            Nice fragment with an open window ! 
            285 $
              | 
             | 
             | 
            	 | 
            	  
	 | 
           
          
            | 
             | 
             | 
             | 
            	 | 
            	 | 
           
          
              
             | 
             | 
             | 
            	 | 
            	
               Sahara 99555-03 
              0.540 gr 
              Nice fragments  
              SOLD
                | 
           
          
            | 
             | 
             | 
             | 
            	 | 
            	 | 
           
            
            | 
             | 
             | 
             | 
            	 | 
            	 | 
             
        
        
        
        
        
        
        
        
        
        
        
         
        
       
       |