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This middle school science passage explores the fascinating world of comets, commonly known as 'dirty snowballs.' Students will learn about the composition and structure of comets, including their icy nuclei and dusty, rocky materials. The reading explains the origins of comets from the Kuiper Belt and Oort Cloud, their highly elliptical orbits, and the dramatic processes that occur as they approach the Sun, leading to the formation of comas and tails. The passage integrates scientific thinking by discussing how space missions like Rosetta have expanded our knowledge. Aligned with NGSS MS-ESS1-2, this resource includes a glossary, comprehension questions, graphic organizers, and is audio-integrated for accessibility. Ideal for grades 6-8, it supports both core and differentiated instruction with English and Spanish translations.
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"The great comet of 1881, observed on the night of June 25-26, at 1h. 20m. A.M." / Library of Congress.
Comets are among the most dynamic and spectacular objects in our solar system. These icy wanderers are sometimes visible from Earth as brilliant streaks of light with glowing tails stretching across the night sky. Scientists study comets to understand the early history of our solar system and the processes that shaped it. Comets help answer questions about the origins of water and organic molecules on planets.
The Structure and Origins of Comets Comets are often described as "dirty snowballs" or "icy dirtballs" due to their unique composition. Their solid center, called the nucleus, is made mainly of ice—such as water, carbon dioxide, methane, and ammonia—mixed with dust and rock. Most comet nuclei are only a few kilometers across, much smaller than planets. Comets come from two main regions: the Kuiper Belt, which is just beyond Neptune and produces short-period comets, and the distant Oort Cloud, the source of long-period comets. These regions act as reservoirs, storing icy bodies that occasionally get nudged toward the Sun by gravitational forces.
Comet Orbits and Their Dramatic Display Comets travel around the Sun in highly elliptical orbits. This means they spend most of their time far from the Sun, moving slowly through deep space. When a comet’s path brings it closer to the Sun, solar heat causes the comet’s ice to undergo sublimation, transforming from a solid directly into a gas. The gas and dust released form a vast, glowing cloud around the nucleus called the coma. The coma can be larger than Jupiter itself. Solar radiation and wind then push this material away from the Sun, creating two distinct tails: a yellowish, curved dust tail and a bluish, straight ion tail. The dust tail is shaped by sunlight, while the ion tail is formed by charged solar particles and always points directly away from the Sun.
Types of Comets and Space Exploration Comets are classified by the length of their orbits. Short-period comets take less than 200 years to orbit the Sun. For example, Halley’s Comet, which has a 76-year orbit, will next return in 2061. Long-period comets can take thousands or even millions of years to complete one orbit and may only visit the inner solar system once in recorded history. Scientific missions, like the European Space Agency’s Rosetta mission, have landed spacecraft on comets to study their surface and composition up close. In 2014, Rosetta’s lander Philae touched down on comet 67P/Churyumov-Gerasimenko, sending back valuable data about its makeup and behavior.
Studying comets gives scientists clues about the conditions that existed when the solar system formed. Because comets are made of ancient material, they act as time capsules preserving information about the distant past. Research on comets could also help us understand how water and organic molecules were delivered to Earth, possibly influencing the development of life. The interactions between comets and the Sun showcase the dynamic processes that shape our solar system.
Interesting Fact: Some comet tails can stretch for millions of kilometers—long enough to span the distance from the Earth to the Moon and far beyond!
What is the main component of a comet's nucleus?
Ice mixed with dust and rockHot gas and plasmaMolten lavaMetal and iron
Where do most short-period comets originate?
Kuiper BeltOort CloudAsteroid BeltJupiter's moons
What happens when a comet gets close to the Sun?
Its ice sublimates, forming a coma and tailsIt explodesIt freezes solidIt disappears
What is the term for the cloud of gas and dust around a comet's nucleus?
ComaCrustMantleAtmosphere
In the passage, what does the word 'sublimation' mean?
Turning from solid to gas without becoming liquidMelting from solid to liquidFreezing from liquid to solidEvaporating from liquid to gas
What does the word 'elliptical' describe in relation to comets?
The shape of their orbitsThe size of their nucleusThe color of their tailThe speed of their movement
Why are comets considered important to study?
They provide clues about the early solar system and origins of waterThey cause eclipsesThey create new planetsThey orbit the Earth
How does the ion tail of a comet behave as it approaches the Sun?
It always points directly away from the SunIt curves toward the SunIt follows the dust tailIt disappears
True or False: All comets return to the inner solar system every 76 years.
TrueFalse
True or False: The Rosetta mission landed on a comet to study it up close.
TrueFalse
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