Meteorite DHO 294-H3.9, polarised LM

Meteorite DHO 294-H3.9, polarised LM

C037/2784 Rights Managed

Request low-res file

530 pixels on longest edge, unwatermarked

Request/Download high-res file

Uncompressed file size: 57.1MB

Downloadable file size: 8.2MB

Price image Pricing

Please login to use the price calculator


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.

Release details: Model release not required. Property release not required.

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

Licence fees: A licence fee will be charged for any media (low or high resolution) used in your project.