*Special Offer: If you would like to have this meteorite classified under your name with our affiliate, the Laboratory for Meteorite Analysis and Classification (LMAC), we will provide the required analysis sample and the 20g type repository sample required for classification at no additional charge. We will also provide you with a $200 discount code for the LMAC classification services which are normally $500 per analysis sample. This offer is only valid if you use LMAC for the analysis and classification services. There is no obligation to classify the meteorite if you purchase it. This is a completely optional value added offer for those who want to take it to the next step. If you do decide to take advantage of this offer, contact us after purchasing the specimen and we will provide more details and instructions on how to proceed with the classification process. 

The Chondrites are undifferentiated meteorites that have not been modified due to melting or differentiation of the parent body. They are formed when various types of dust, water ice, small mineral grains, chondrules and chondrule fragments present in the early solar system accreted to form primitive asteroids. They are the most common type of meteorite that falls to Earth with estimates for the proportion of the total fall that they represent varying between 85.7% and 86.2%, with most of those chondrites being equilibrated ordinary chondrites, often referred to as simply ordinary chondrites (OC) or equilibrated chondrites (EC). The Ordinary Chondrites come in three types (LL, L, and H) depending on the iron content of their olivine and pyroxene. Each of these three types are then given petrological grades between 3 and 7 depending on how equilibrated they are, with 3 being the least equilibrated and 7 being the most equilibrated. There are several less common types of chondrites including; Carbonaceous Chondrites (C), Enstatite Chondrites (E), Rumuruti-like Chondrites (R), and Kakangari-like Chondrites (K). The study of the ordinary chondrites and the other types of chondrites provides important clues for understanding the origin and age of the Solar System, the synthesis of organic compounds, the origin of life, and how Earth got its water. One of the key characteristics of the chondrites is the presence of chondrules, which are complex spherical mineral grains, often glassy and having gone through multiple rapid heating events. Chondrules typically constitute between 20% and 80% of a chondrite by volume.

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