
Fragment of Chelyabinsk meteor currently being analyzed for mineral composition and signs of previous melting.
The Chelyabinsk meteor, estimated to have been 55-65 feet in diameter before breaking up, may have had previous fiery encounters — either colliding into another body in the solar system or traveling too close to the Sun — before its spectacular crash to Earth, according to analysis of fragments from its crust and interior.
Hints of Heat
Presenting the new findings at a geochemical conference today in Florence, Italy, Victor Sharygin of Novosibirsk's Institute of Geology and Mineralogy said a detailed mineral analysis of fragments of the meteorite revealed some anomalies suggesting the rock had previously been melted.
Dividing the pieces into different gradations of color and structure, the team identified a concentration of dark fragments composed of fine-grained material formed by extremely intense melting. The dark fragments were distinct from the meteorite's fusion crust, a thin layer that melts and then solidifies as the rock travels through Earth's atmosphere. The dark fragments' structure included what the team described as "spherical bubbles," either encrusted with oxide, silicate and metal or filled with metal and sulfide.














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