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دنباله‌دار

File:Comet_Hale-Bopp_1995O1.jpg · Wikimedia Commons · See Wikimedia Commons

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دنباله‌دار

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A comet is an icy, small Solar System body or interstellar object that warms and begins to release gases when passing close to the Sun, a process called outgassing. This produces an extended, gravitationally unbound atmosphere or coma surrounding the nucleus, and sometimes a tail of gas and dust gas blown out from the coma. These phenomena are due to the effects of solar radiation and the outstreaming solar wind plasma acting upon the nucleus of the comet. Comet nuclei range from a few hundred meters to tens of kilometers across and are composed of loose collections of ice, dust, and small roc

AI overview

A comet is a small, icy body from the Solar System that releases gases and dust when it travels near the Sun, creating a glowing atmosphere and sometimes a visible tail. Comets matter because they are natural objects that demonstrate how solar radiation and wind affect matter in space, and their appearance in our sky has made them historically significant to observers on Earth.

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Key facts

Astronomical formation.image
File:Comet Hale-Bopp 1995O1.jpg
Astronomical formation.caption
Comet Hale–Bopp after passing perihelion in April 1997
Astronomical formation.thing
Small solar system body
Astronomical formation.where
Star systems
Astronomical formation.density
0.6 g/cm3 (average)
Astronomical formation.qid
Q3559
Astronomical formation.commonscat
Comets
Astronomical formation.size
Typically less than 10 km wide (nucleus)
Astronomical formation.Mass
1011 kg to 1017 kg

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