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After a meteoroid breaks up, the largest fragments travel a little farther because they have greater momentum. This stamp depicts the shower in Jilin, China.
When a meteoroid enters the Earth's atmosphere, it is subjected to enormous stress. This is due to the difference in pressure at the front and the back of the object and the differences in temperature between its surface and its core. Large stony meteoroids do not hold up well to these stresses and break easily.

Fragmentation takes place at low altitude, and the fragments fall together to the ground, forming an ellipse. The largest fragments are usually found at the front of the ellipse and indicate the direction of the fall. A shower can total several tens, hundreds, or thousands of fragments. After a shower rained down on the village of Pultusk in Poland in January 1875, more than 100,000 fragments were recovered! Besides showers from the fragmentation of one meteoroid, multiple falls can be caused by meteoroids travelling together in space.

SOME IMPORTANT METEOR SHOWERS
Name Country Year Number of fragments
 Allende  Mexico 1969 Thousands
 Sikhote-Alin  Russia 1947 Thousands
 Pultusk  Poland 1868 Between 100,000 and 300,000
 Holbrook  United States 1912 16,000
 L'Aigle  France 1803 Between 2,000 and 3,000
 Bruderheim  Canada 1960 700
 Homestead  United States 1875 100


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Fragments from the Pultusk meteorite in Poland, spread out in an ellipse measuring 8 kilometres by 1.6 kilometres.

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Fragments from the shower in Mbale, Uganda, vary in size from 0.1 gram to 27.4 kilograms.


Fragmentation of the Peekskill meteoroid captured on video by a spectator at a football game.

© O. Shinfineld, Halifax, Virginia

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Credits.  Last Modified: 2005-09-30