Description: A meteorite is a solid cosmic body between 30 micrometers and 1 meter in size that falls to the surface of the Earth or another celestial body after passing through that body's atmosphere. An object is only described as a meteorite after it has passed through the Earth or other celestial body's atmosphere. While in interplanetary space and while it is passing through the atmosphere it is known as a meteoroid. The shock wave the meteoroid causes in the atmosphere emits light and may be observed as a meteor.

Meteorites are usually made of stone, iron-stone, or iron, with stone being the most common when we look at types of meteorites that are linked to the sighting of a meteor. However, stony meteorites often look like terrestrial rocks so can be overlooked and iron meteorites are the most common type of meteorite found on the ground. Most meteorites are found in Antarctica or deserts as this is where they are easiest to spot.

Most of the found meteorites range from a few grams to several kilograms in mass. The largest known one is Hoba, which is more than 60 tons and lies in Namibia. Some meteorites can be large enough to produce an impact crater. Meteorites are named after the area where they fell.

Related Terms:

• Iron Meteorite
• Meteoroid
• Shooting Star

Term and definition status: This term and its definition have been approved by a research astronomer and a teacher

The OAE Multilingual Glossary is a project of the IAU Office of Astronomy for Education (OAE) in collaboration with the IAU Office of Astronomy Outreach (OAO). The terms and definitions were chosen, written and reviewed by a collective effort from the OAE, the OAE Centers and Nodes, the OAE National Astronomy Education Coordinators (NAECs) and other volunteers. You can find a full list of credits here. All glossary terms and their definitions are released under a Creative Commons CC BY-4.0 license and should be credited to "IAU OAE".