A Journey Through Our Solar System's Debris

Discover the distinct characteristics of comets, asteroids, and meteors. Click on the facts below to reveal more information and explore the interactive simulation.

Comets

Often called "dirty snowballs," comets are cosmic bodies of frozen gases, rock, and dust. They originate in the far reaches of our solar system and are known for their spectacular tails.

Composition: Ice and Dust

A comet's core, or nucleus, is a mixture of water ice, frozen gases like carbon dioxide, methane, and ammonia, mixed with rock and dust.

Orbit: Highly Elliptical

Comets have long, stretched-out orbits that bring them very close to the Sun and then fling them out to the solar system's edge. This is why we only see them periodically.

The Tail: A Solar Phenomenon

As a comet nears the Sun, its ice vaporizes, creating a glowing cloud called a coma and two tails: a bright dust tail and a bluish ion tail. The tails always point away from the Sun due to solar wind.

Interactive Solar System Simulation