Article
Article
Meteor
Article By:
Meisel, David D. Department of Physics and Astronomy, State University of New York, Geneseo, New York.
Last reviewed:December 2019
DOI:https://doi.org/10.1036/1097-8542.420400
- Visual observation
- Physical characteristics
- Meteoroid orbits and velocities
- Origins of shower meteors
- Photographic and electronic observations
- Radio and radar observations
- Nontraditional meteor studies and research
- Leonids in 1996–2003
- Scientific results from the Leonids
- Related Primary Literature
- Additional Reading
The luminous streak lasting seconds or fractions of a second and seen at night when a solid, natural body plunges into the Earth's (or another planet's) atmosphere. The entering object is called a meteoroid and, if any of it survives atmospheric passage, the remainder is called a meteorite. Cosmic dust particles (with masses of micrograms) entering the atmosphere and leaving very brief, faint trails are called micrometeors, with the surviving pieces known as micrometeorites. If the apparent brightness of a meteor exceeds that of the planet Venus as seen from Earth, it is called a fireball; and when a bright meteor is seen to explode, it is called a bolide. See also: Meteorite; Micrometeorite
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