Meteorite identification involves several key tests to distinguish them from terrestrial rocks.
Visual Examination.
As with any field of expertise, people who are highly experienced in understanding and handling confirmed meteorites will understand key traits and features to look for when examining a specimen.
Fusion Crust Examination.
This is is essential, as meteorites often have a thin, dark, glassy crust formed during atmospheric entry.
Regmaglypt Surface Examination.
Regmaglypts are thumbprint-like impressions on the surface are also characteristic of meteorites.
Density Test.
Meteorites are generally denser than Earth rocks due to their metal content.
Streak Test.
The sample is rubbed on unglazed porcelain; meteorites typically leave no streak, unlike many Earth rocks.
Magnetic Test.
Most meteorites contain iron-nickel metal, making them magnetic. However, not all meteorites are strongly magnetic, so this test is not definitive.
Interior Examination.
This can reveal a metallic, grainy texture with chondrules or metal flakes, which are indicative of meteorites.
Advanced tests include;
These tests, usually conducted in specialized laboratories, are essential for accurate meteorite identification.
For more detailed methodologies, refer to resources from institutions like the University of Arizona's Lunar and Planetary Laboratory or the Meteoritical Society's publications.