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Comparing the Planets

Interactive passage with audio narration, comprehension questions, and printable PDF.

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Format: Interactive (Online), Printable (PDF)
Grades: 5678
Subjects: sciencereadingela
Standards: MS-ESS1-2
Languages: English, Spanish

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Reading passage

Reading comprehension

Audio narration

With word word highlighting

Comprehension quiz

Auto-graded

Writing activity

Open-ended response

Glossary & flashcards

Vocabulary practice

Differentiated version

Adapted for varied levels

Spanish translation

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About this reader

This informational science passage for grades 6-8 aligns with NGSS standard MS-ESS1-2 and provides a comprehensive comparison of the planets in our solar system. Students will learn how planets are grouped based on composition—terrestrial, gas giants, and ice giants—and how features like atmosphere, size, density, and temperature differ among them. The passage emphasizes scientific thinking, showing how data such as mass, density, and day length help scientists classify and understand planetary systems. Real-world applications are highlighted, including how planetary characteristics affect exploration and technological challenges. Activities include multiple-choice questions, writing prompts, and graphic organizers, all with audio integration for accessibility. This resource helps students connect planetary science to broader scientific principles, supporting critical thinking and analysis in line with MS-ESS1-2. Keywords: planets, solar system, terrestrial, gas giants, ice giants, density, atmosphere, grade 6-8 science.

Written by Workybooks TeamPublished by Workybooks

Sample passage and quiz content

CONTENT PREVIEW

"Kepler 51 planets compared to some of the planets in our Solar system" by NASA, ESA, and L. Hustak and J. Olmsted (STScI) /
Source: Wikimedia Commons (Public domain).

Planetary science allows us to organize the planets of our solar system into groups based on their physical characteristics. When scientists observe the night sky, they notice that not all planets are alike. Some are small, rocky, and dense, while others are enormous and made mostly of gases. Understanding these differences helps reveal how planets form and interact as systems.

Types of Planets and Their Features
The four terrestrial planets—Mercury, Venus, Earth, and Mars—share several characteristics. They are all rocky, have solid surfaces, and are relatively small and dense (about 5 grams per cubic centimeter). These planets have few or no moons, and their atmospheres vary: Venus has a thick, toxic atmosphere, Mars has a thin one, and Mercury has almost none at all. Earth's atmosphere supports life and regulates temperature. Surface conditions among terrestrial planets are influenced by atmosphere; for example, Mercury's lack of atmosphere causes extreme temperature swings from 430°C during the day to -180°C at night.

Gas Giants and Ice Giants
Jupiter and Saturn are known as gas giants. They are much larger than terrestrial planets, mostly composed of hydrogen and helium, and have no solid surface. Their low densities, especially Saturn’s (which would float in water), result from their gaseous composition. Both have many moons and ring systems. Uranus and Neptune are ice giants, somewhat smaller than gas giants but with significant differences. Their atmospheres contain more ices like water, ammonia, and methane, which gives Neptune and Uranus their blue color. Methane absorbs red light and reflects blue, making these planets stand out. Ice giants also have many moons and faint rings.

Comparing Size, Density, and Motion
The solar system’s planets show dramatic variety in size and mass. Jupiter is the most massive, about 318 times Earth’s mass, while Mercury is the smallest at only 0.055 times Earth’s mass. Densities also vary: Earth is the densest planet, while Saturn is the least dense. Day lengths differ, too. Venus rotates very slowly, taking 243 Earth days for one rotation, while Jupiter spins quickly in about 10 hours. A planet’s orbital period, or year, is also different: Mercury takes just 88 Earth days, but Neptune’s year lasts 165 Earth years. These variations are measured using telescopes and space probes, which collect data about each planet’s movement, size, and composition.

Studying planetary differences helps scientists understand the processes that shape planet formation and evolution. It also guides future space missions and the search for life beyond Earth by focusing on planets with conditions that might support life.

Interesting Fact: Saturn is so light for its size that it would float in water—if you could find a bathtub big enough!

Which group of planets is known for having rocky surfaces and high density?

Terrestrial planetsGas giantsIce giantsDwarf planets

What causes the blue color of Uranus and Neptune?

Hydrogen in the atmosphereMethane absorbing red lightIron on the surfaceThick oxygen clouds

Which planet would float in water because of its low density?

SaturnEarthMarsMercury

How do scientists measure the differences between the planets?

By using telescopes and space probesBy listening for soundsBy tasting samplesBy guessing from pictures

What does the term "orbital period" mean in the passage?

The time it takes a planet to rotate onceThe time it takes a planet to orbit the SunThe temperature of a planetThe number of moons a planet has

Why do terrestrial planets have more extreme temperature changes compared to gas giants?

Because they have thin or no atmosphereBecause they have more moonsBecause they are made of gasBecause they are farther from the Sun

Which is true about gas giants and ice giants?

They all have many moons and ring systemsThey have solid rocky surfacesThey are smaller than terrestrial planetsThey have only one moon each

If a new planet is discovered with a thick methane atmosphere and many moons, which group would it likely belong to?

Terrestrial planetsDwarf planetsGas giantsIce giants

Jupiter is more massive than Earth.

TrueFalse

Mercury has a very thick atmosphere.

TrueFalse

Comparing the Planets

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