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Lesson

Sun-Earth-Moon System

Three objects. One invisible force. An elegant balance that has held for billions of years — and makes life on Earth possible.

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Driving Question
Why don't Earth and the Moon just fly apart or crash together?
🔬 Learning Science Focus 🔍 Phenomenon-First 🧠 Chunked Content 🔗 Analogical Reasoning ✅ Retrieval Practice
📋 MA STE Standards · Grade 6 MS-ESS1-1 MS-ESS1-2
MS-ESS1-1 Develop and use a model of the Earth-Sun-Moon system to describe the cyclic patterns of lunar phases, eclipses of the Sun and Moon, and seasons.
MS-ESS1-2 Explain the role of gravity in the motions within galaxies and the solar system; understand that orbital periods and speeds are determined by gravitational forces between objects.

Something Doesn't Add Up

Before we explain anything — just think. You've seen the first thing happen thousands of times. The second one has been happening for 4.5 billion years.

DROP A BALL It hits the ground. vs. THE MOON Earth moving sideways pulled down It never hits. Why?

Gravity pulls the Moon toward Earth — just like it pulled that ball. So why hasn't the Moon crashed into Earth in 4.5 billion years?

The Sun-Earth-Moon System

Three objects — a star, a planet, and a moon — held in perfect balance by gravity and motion. Here is how it all works.

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Surprising Scale Fact

Same Size. Completely Different.

Look up on a clear night and the Sun and Moon appear almost exactly the same size in the sky. But the Sun is 400 times larger than the Moon. The reason they look identical is that the Sun is also almost exactly 400 times farther away. This remarkable coincidence is what makes total solar eclipses possible — the Moon fits almost perfectly over the Sun's face. Understanding how three objects at such wildly different scales can interact so precisely starts with understanding the force that holds them together: gravity.

👆 Click any card below to read the full notes for that topic.

What Is a System?
A group of parts that interact and affect each other — the Sun, Earth, and Moon are one system.

A system is a group of parts that interact with and affect each other. The Sun, Earth, and Moon form one system — connected by gravity and motion. Change one part of the system and the rest responds.

System
A group of parts that interact with and affect each other. The Sun-Earth-Moon system has three members: a star (the Sun), a planet (Earth), and a natural satellite (the Moon). All three are connected by gravity and held in their paths by the balance between gravity and forward motion.
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What holds it together? Remove Earth's forward speed and it spirals into the Sun. Remove the Sun's gravity and Earth flies off into space in a straight line. The system only works because both forces — gravity and motion — are always present and balanced.
What Is Gravity?
An invisible pulling force between objects with mass — it holds the entire system together.

Gravity is an invisible pulling force between any two objects that have mass. It always pulls toward the center of a massive object, which is why every person on Earth — no matter where they are standing — feels pulled straight down toward Earth's core.

Gravity
An invisible pulling force between any two objects that have mass. Gravity always pulls toward the center of a massive object. Albert Einstein described gravity not as a force but as the warping of spacetime — massive objects bend the fabric of space, and other objects follow those curves. For our purposes, gravity is the invisible thread that holds the Sun-Earth-Moon system together.
Mass
The amount of matter in an object. More mass = stronger gravitational pull. The Sun contains over 99% of all mass in the solar system, giving it enough gravity to hold all eight planets in orbit. The Moon's mass is much smaller — its surface gravity is only about 1/6 of Earth's, which is why astronauts could bounce easily on its surface.
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Tug-of-war analogy: Think of gravity like a tug-of-war. A heavier person pulls harder — bigger mass, bigger pull. The Sun is so massive it wins the tug-of-war with all eight planets at once, holding every one of them in orbit.
Earth Orbits the Sun
One full orbit takes 365.25 days — gravity and forward speed working together create a stable path.

Earth travels in a nearly circular path around the Sun called an orbit. One full trip around the Sun takes about 365.25 days — that 0.25 is why we add a Leap Day every four years. Earth's speed along this path is roughly 67,000 mph.

Orbit
The curved path one object takes around another due to gravity. Earth's orbit around the Sun is nearly circular — a shape called an ellipse. The Sun's gravity continuously pulls Earth inward; Earth's forward speed continuously tries to carry it away. The result is a stable curved path.
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Why curved and not straight? Without the Sun's gravity, Earth would travel in a straight line into deep space. Without Earth's forward speed, Earth would fall straight into the Sun. The orbit exists because gravity and speed balance each other — the Sun's pull curves Earth's straight-line motion into a loop.
The Moon Orbits Earth
Earth's only natural satellite orbits every 27–29 days, held in place by Earth's gravity.

The Moon is Earth's only natural satellite. It orbits Earth in about 27–29 days — roughly one month. Earth's gravity holds the Moon in orbit, in exactly the same way the Sun's gravity holds Earth in orbit.

Natural Satellite
A natural object (not built by humans) that orbits a planet, held in place by the planet's gravity. Earth has one natural satellite — the Moon. Some planets have many: Saturn has over 140 known moons. A satellite that humans build and launch into orbit is called an artificial satellite.
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The same relationship, nested: The Sun's gravity holds Earth in orbit. Earth's gravity holds the Moon in orbit. The Moon does not orbit the Sun directly — it orbits Earth, which orbits the Sun. All three are locked together in one system.

Rotation vs. Revolution

Two words, two completely different kinds of motion — and one of the most common mix-ups in middle school science. Here is how to keep them straight.

The 4 Key Rules

1
Rotation = spinning on an axis. Earth rotates on its own internal axis — an imaginary line running through the North and South Poles — once every 24 hours.
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Revolution = traveling along an orbit. Earth revolves around the Sun — one full trip — every 365.25 days. This produces our year.
3
Rotation produces day and night. As Earth spins, different parts of its surface face the Sun (daytime) or face away from it (nighttime).
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Both move counterclockwise. Viewed from above Earth's North Pole, both Earth's rotation and its revolution around the Sun move counterclockwise.

Side by Side

Feature Rotation Revolution
Definition Spinning on an axis Traveling around another object
Earth's period ~24 hours ~365.25 days
What it produces Day and night The year
Direction Counterclockwise Counterclockwise
Key words Spin · Axis · Day Orbit · Year · Path

Sun, Earth, and Moon

Three very different objects, bound into one system. Click any card to read the key facts — then explore the Motion Explorer to see rotation and revolution in action.

👆 Click each card to expand its key facts. Then use the Motion Explorer below to see rotation and revolution visualized.
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The Sun
Star
The gravitational anchor of the system. The Sun is an average-sized yellow star about 4.6 billion years old. Its enormous mass — over 99% of all mass in the solar system — generates the gravity that holds Earth and all seven other planets in orbit. About 1 million Earths could fit inside it. It is approximately 110 times the diameter of Earth and sits about 93 million miles from us.
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Earth
Planet
The third planet from the Sun, and the only known world with liquid water on its surface. Earth orbits the Sun once every 365.25 days at roughly 67,000 mph. It also spins on its tilted axis every 24 hours, creating day and night. Earth is about 4 times wider than the Moon — much larger than the Moon appears from Earth's surface. Its atmosphere blocks harmful radiation and keeps temperatures stable.
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The Moon
Natural Satellite
Earth's only natural satellite — about 240,000 miles away. The Moon completes one orbit around Earth every 27–29 days. Earth's gravity holds it in orbit. The Moon's surface gravity is 1/6 of Earth's, which is why astronauts bounced on its surface. Despite being 400 times smaller than the Sun, the Moon appears nearly the same size in our sky because it is also 400 times closer — which is why total solar eclipses are possible.
Motion Explorer
Toggle between rotation and revolution to see each type of motion visualized.
Earth: 1 Revolution = ~365.25 Days  ·  Moon: ~27–29 Days Both orbit counterclockwise (viewed from above North Pole)
Earth's Rotation
One full spin on Earth's tilted axis (23.5°) takes 24 hours — creating day and night. The continents spin counterclockwise when viewed from above the North Pole. The axis stays fixed in space while Earth spins around it.

Vocabulary to Know

Every term below appeared in this lesson. Click any pill to jump to its explanation.

👆 Click any term to jump to its explanation in the lesson

System Gravity Mass Orbit Natural Satellite Rotation Revolution Axis Model

Reflect Before You Quiz

Three questions — no grade, no pressure. Just think it through before the quiz.

Earth completes one full spin every 24 hours and one full orbit around the Sun every 365 days. Which of these is its rotation?

If Earth's gravity suddenly switched off, what would happen to the Moon?

From Earth, we always see the same face of the Moon — the far side was never photographed until a spacecraft flew around it. What does this tell us about the Moon?

Sun-Earth-Moon Quiz

10 questions on gravity, orbits, and the motions of our solar system's closest neighbors. Fill in your info below — your score will be sent to your teacher when you submit.

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More Learning

The lesson is just the beginning — go deeper, see the next lesson in the unit, or explore NASA's real data.