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Mercury: Closest to the Sun

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-ESS1-2MS-ESS1-3
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 comprehensive, standards-aligned passage explores Mercury—the smallest and closest planet to the Sun. Students in grades 6-8 discover Mercury’s orbit, rotation, extreme temperature swings, and unique features such as the Caloris Basin and massive scarps. The text explains how Mercury’s weak exosphere and large iron core contribute to its characteristics, and highlights key scientific discoveries from spacecraft like Mariner 10 and MESSENGER. Students learn about cause-and-effect relationships, surface processes, and planetary systems, connecting these to NGSS standards MS-ESS1-2 and MS-ESS1-3. Audio integration supports diverse learners, while accompanying activities deepen comprehension and critical thinking. This resource is ideal for engaging middle school learners in planetary science and the mechanisms shaping our solar system.

Written by Workybooks TeamPublished by Workybooks

Sample passage and quiz content

CONTENT PREVIEW

"Planet Mercury - GPN-2000-000465" by NASA/JPL/USGS /
Source: Wikimedia Commons (Public domain).

Mercury is the smallest planet in our solar system, with a diameter of only 4,880 kilometers—just slightly larger than Earth's Moon. As the planet closest to the Sun, Mercury is located about 0.4 astronomical units (AU) from our star. This proximity has major effects on Mercury’s environment, making it a fascinating example for scientists studying how planets form and change.

Speedy Orbit, Slow Rotation
Mercury’s orbit is the fastest of all the planets, completing one trip around the Sun in only 88 Earth days. However, Mercury rotates slowly on its axis, taking about 59 Earth days to spin once. Because of a phenomenon called orbital resonance, Mercury rotates three times for every two orbits around the Sun. This means a single day, from sunrise to sunrise, lasts 176 Earth days! These unique movements create long, hot days and equally long, freezing nights.

Surface Features and Extreme Temperatures
Mercury’s surface is heavily cratered, resembling the Moon because it lacks significant weather or erosion. The planet’s most striking feature is the Caloris Basin, a colossal impact crater stretching 1,550 kilometers across—nearly a third of Mercury’s diameter. Mercury also has gigantic scarps, or cliffs, which formed as the planet cooled and contracted over time. Without a thick atmosphere, Mercury cannot retain heat. Instead, it has a thin exosphere, made up of atoms knocked off the surface by the solar wind. As a result, temperatures swing dramatically, from 430°C (800°F) during the day to -180°C (-290°F) at night—the largest temperature range of any planet.

Internal Structure, Magnetic Field, and Exploration
Mercury contains a massive iron core, which makes up about 60% of its mass and helps generate a weak magnetic field. Scientists have learned about Mercury’s structure and surface by observing it from Earth and sending spacecraft, such as Mariner 10 in the 1970s and MESSENGER from 2011 to 2015. These missions used cameras and instruments to map the surface, measure the magnetic field, and analyze the exosphere. Observing Mercury is challenging because it always appears close to the Sun from Earth, but astronomers look for it when it is at its greatest elongation—its farthest point from the Sun in our sky.

Mercury’s extreme conditions and surface features reveal much about the processes that shape rocky planets. By studying Mercury, scientists gain insight into planetary formation, internal structure, and the impact of solar energy on planetary bodies. Understanding Mercury helps us better grasp the complex systems at work in our own solar system and beyond.

Interesting Fact:
On Mercury, a single day from sunrise to sunrise is twice as long as its year!

Which planet is closest to the Sun?

MercuryVenusEarthMars

What is the diameter of Mercury?

4,880 kilometers12,742 kilometers6,371 kilometers1,550 kilometers

What is the Caloris Basin?

A huge impact crater on MercuryA type of cloud on MercuryA volcano on MercuryA moon of Mercury

Which best describes 'scarps' on Mercury?

Steep cliffs formed as the planet cooled and shrankRivers on Mercury's surfaceWinds that blow across MercuryCraters formed by asteroids

What is Mercury’s atmosphere like?

It has a very thin exosphere, almost no atmosphereIt has thick clouds and strong windsIt is full of water vaporIt is mostly nitrogen and oxygen

What does 'orbital resonance' mean in the passage?

Mercury rotates three times for every two orbits around the SunMercury and Venus move at the same speedMercury’s orbit changes direction each yearMercury always faces the Sun

Why does Mercury have such extreme temperature changes?

It has no thick atmosphere to hold in heatIt is covered with iceIt spins very quicklyIt is far from the Sun

How have scientists learned about Mercury’s surface and core?

By sending spacecraft and using telescopesBy visiting Mercury in personBy studying Mercury’s moonsBy measuring the air on Mercury

True or False: Mercury’s day is shorter than its year.

FalseTrue

True or False: Mercury is easy to see in the night sky.

FalseTrue