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An engaging introduction to comets, asteroids, and meteors, explaining their differences, characteristics, and origins. Students will learn about the various parts of a comet, the difference between meteoroids, meteors, and asteroids, and the orbits and compositions of these celestial bodies. The document also includes interactive activities, such as watching Comet ISON's path and completing a Venn diagram, to help students better understand the concepts.
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Comets and Asteroids and Meteors, Oh My! Comets
The sight of a falling star is exciting. Before you can say, “Look!” the streak is gone. You point to where it was and ask others if they saw it, too. Often, no one else sees the speedy flight of light flash by. You’re left trying to describe what you saw and felt. You stare at the dark space, hoping another will streak across the sky. What is a falling star? A falling star is not a star at all. It is not even a piece of a star. Stars are huge balls of burning gas sending off great amounts of energy in the form of light and heat. Stars are much bigger than our planet. Stars do not fall; they stay in their own places in their own galaxies. Our Sun is a star. A falling star is a meteor. Meteors are streaks of light in the sky that we can see when a small speck of dust burns up high in the air above us. Where do these specks of dust come from? Comets! (And, don’t forget space dirt!) Astronomers call this dirt and comet dust “ meteoroids .” Meteoroids are different sizes. Some are larger. Most are tiny. Meteoroids hit the Earth’s atmosphere at super, high speed. Sometimes it’s faster than 90,000 miles per hour. When they are in the atmosphere, they become “ meteors .” The meteor usually burns up. This creates the streak of light we see. It looks like a star falling from the sky. This is why they are called a “falling star.” Meteors usually last just a second or two.
Characteristics to include in the Venn Diagram: