Nucleus: This is the solid, central part of the comet, made up of ice and rock.
Coma: As a comet gets closer to the Sun, its ice begins to vaporize and forms a cloud of gas and dust around the nucleus, called the coma.
Tail: The solarwind and radiation pressure from the Sun push the gas and dust away from the coma, forming a tail that can stretch for millions of kilometers.
Comets have highly elliptical orbits, which means they can spend most of their time in the distant reaches of the solar system before swinging in close to the Sun. Many comets come from the Kuiper Belt and the Oort Cloud, which are regions beyond the orbit of Neptune that contain icy bodies left over from the formation of the solar system.
Study Guide
Here are some key points to remember when studying comets:
Earth's surface changes constantly through a variety of processes and forces. Students can:
Analyze and interpret data identifying ways Earth's surface is constantly changing through a variety of processes and forces such as plate tectonics, erosion, deposition, solar influences, climate, and human activity
Develop and communicate an evidence based scientific explanation around one or more factors that change Earth's surface