A comet is an icy, small Solar System body that warms and begins to release gases when passing close to the Sun, a process called outgassing.
Overview
How Comets Form
What Is A Comet
Orbits And Pathways
Observation Techniques
Famous Comets In History
Composition And Structure
Cultural Significance Of Comets
Comet Vs Asteroid Key Differences
The Role Of Comets In Planetary Science
Hubble Space Telescope
Halley's Comet
Imagination
Information
Kuiper Belt
Solar Wind
Asteroid
Planet
Space
Eye
๐ Comets are icy bodies that travel through space and have a glowing tail when close to the Sun.
โ๏ธ A comet is like a dirty snowball made of ice, rocks, and gas.
๐ Some comets can be over 4.6 billion years old, almost as old as our Solar System!
๐ The gas and dust released by a comet form a spectacular glowing tail that can stretch for millions of kilometers.
๐ Comets have three main parts: the nucleus, the coma, and the tail.
๐ซ๏ธ The coma around the nucleus can be thousands of kilometers wide and glows brightly.
๐ Comets can come from areas like the Kuiper Belt and the Oort Cloud.
๐ A famous comet, Halley's Comet, visits us every 76 years and was last seen in 1986.
๐ญ Astronomers use telescopes to study and capture images of comets in the night sky.
๐ง Studying comets helps scientists learn about the origins of water on Earth and the early Solar System.
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