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                Similarities & Differences - 
                L3 & LL3 Chondrites When studying NWA 3099 (L/LL3) 
                it is evident that there are numerous unusual inclusions within 
                the matrix. 
                When comparing this meteorite with NWA 864 (L3.3) there are 
                notably similar inclusions present. These are the mottled 
                greyish inclusions which contain much smaller (~0.1-0.2mm) paler 
                inclusions inside. I have discussed this with fellow collector, 
                Bernd Pauli who came up with some very interesting theories. 
                This is what Bernd had to say about NWA 3099: "While rare; it may be possible that this 
                meteorite contains Carbonaceous inclusions. A well-known example 
                is Krymka (LL3.1/S3) some slices of which include black 
                carbonaceous material, referred to as 'Mysterite'. 
                Interestingly, where there is Mysterite in the Krymka chondrite, 
                there is also abundant Troilite (Iron Sulphide) in the matrix. There are also 
                graphite-bearing fragments and, again, these fragments contain a 
                high abundance of Troilite and graphite.
 Maybe NWA 3099 is as, or, at least almost as "primitive" as 
                Krymka or even Semarkona and thus would contain material from the early 
                days of our solar system. Like in Krymka, the C-rich clasts might be of a 
                pre-accretionary nature, and maybe there are even presolar nanodiamonds like the 
                ones that have been reported from Krymka. Maybe there is even a relation 
                to cometary material as has been assumed for Krymka carbonaceous material."
 
                Even though the overall matrix of NWA 3099 is reasonably pale in 
                colour, I have since found similar 
                mottled features in NWA 1933 (LL3) which has a much darker 
                appearance. Bernd also immediately 
                recognized the same dark matrix, many crisp chondrules and 
                inclusions of NWA 864 (L3.3) as is evident in Krymka (LL3.1). On 
                further checking, the Meteoritical Bulletin actually makes 
                special note that NWA 864 is Highly Unequilibrated and thus 
                probably has a petrologic grade lower than the official level of 
                L3.3. It also says that its matrix contains fine blades and 
                laths of Iron rich olivine and is very similar to the Krymka 
                (LL3.1) matrix. 
                When viewing these different Type-3 Chondrites, it seems 
                relatively comprehensible to assume that there may indeed be one 
                common source (parent 
                body) or a number of related sources in which 
                these incredible primordial meteorites originated. 
                
                
 
                
                 Mottled Grey / 
                White Inclusion in NWA 3099.
 
                
                NWA 3099
                (L/LL3) -  11.80g Complete Slice. 
 
                %207.60g%20(2%20of%202).jpg) NWA 1933
                (LL3) -  7.60g Complete Slice.
 
                
                 NWA 864
                (L3.3) - 7.60g Endcut.
 
                
                 Krymka (LL3.1) - 6.80g Complete Slice. (Bernd Pauli Collection)
 
                
                 Krymka
                (LL3.1) - 5.58g Complete Slice. (Peter Marmet Collection)
 
                
                 Dho 008
                (L3.2-3.3) - 2.20g Partslice.
 
                
                 Sahara 98175
                (LL3.5) - 3.94g Endcut.
 
                
                 Moorabie
                (L3.8) - 0.256g Partslice.
 
                
                .jpg) NWA 
                2288
                (L3) - 9.41g Slice.
 
                  
                  
                
                
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