Meteoroid

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Meteoroid

A meteoroid is a small rocky or metallic body in outer space. Meteoroids are significantly smaller than asteroids, and range in size from small grains to one-meter-wide objects. Most are fragments from comets or asteroids, whereas others are collision impact debris ejected from bodies such as the Moon or Mars.

Formation[edit | edit source]

Meteoroids are formed from the collision of asteroids and by the disruption of comets. They are also formed from the debris ejected during the formation of the Solar System.

Classification[edit | edit source]

Meteoroids are classified into three main types: iron, stony, and stony-iron. Iron meteoroids are largely composed of iron and nickel. Stony meteoroids are made up of silicate minerals, while stony-iron meteoroids are a mixture of metallic and rocky material.

Effects on Earth[edit | edit source]

When a meteoroid enters the Earth's atmosphere, it begins to ablate and creates a bright streak of light known as a meteor. If a meteoroid reaches the ground and survives impact, then it is called a meteorite.

See also[edit | edit source]

References[edit | edit source]


Meteoroid Resources
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Contributors: Prab R. Tumpati, MD