Meteorite DHO 294-H3.9, polarised LM

Meteorite DHO 294-H3.9, polarised LM

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Credit: ALFRED PASIEKA/SCIENCE PHOTO LIBRARY

Caption: Polarised light micrograph of a thin section microscopic slide of the DHO 294_H3.9 chrondite type meteorite, found 2004 in the region of Dohar/Al Wusta, Oman. Chondrites are stony (non-metallic) meteorites that have not been modified due to melting or differentiation of the parent body. They are formed when various types of dust and small grains that were present in the early solar system accreted to form primitive asteroids. They are the most common type of meteorite that falls to Earth. Horizontal object size of this section: 1.2 mm.

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Keywords: al wusta, asteroids, astronomical, astronomy, chondrite meteorite, composition structure, cosmological, cosmology, dho 020, dohar, extraterrestial, light micrograph, meteor, meteorite, meteoroide, meterorid, oman, solar system, stony, thin section

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