Meteorite strewnfield
impactor that breaks up in the atmosphere but does not fully vaporise From Wikipedia, the free encyclopedia
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A meteorite strewnfield is the area where meteorites and glassy tektites from a single meteor fall are found.[1][2][3]

Formation
There are two ways for strewnfields to form:
- Mid-air fragmentation. When a large meteor enters the atmosphere it often fragments into many pieces. This showers the material over a large oval-shaped area. The shape of this oval is caused by the flight path of the meteor. When multiple-explosions occur, the material may be found in several overlapping ovals.
- Impact fragmentation: the fragmentation can occur on impact. In this case the strewnfield shape may be different, usually circular.
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Example
- The Australasian strewnfield is the youngest and largest of the tektite strewnfields. Recent estimates suggest it may cover 10%-30% of the Earth's surface.[4]
References
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