Why Do Tides Happen?

The Moon, the Ocean, and a Hidden Force That Moves Our Shores

You Picked the Perfect Spot. Then the Ocean Moved.

You got to the beach early and claimed your spot near the water. Umbrella planted. Towel laid out. Sun on your face. You doze off to the sound of waves. An hour later, you wake up nearly underwater. This happens every day, all over the world. The ocean quietly rises and falls, like it’s breathing. But why?

Most people say, “It’s the moon.” But that’s not an answer—that’s just the beginning. If the moon controls the tides, why are they strongest during a full moon? Why do we get two high tides a day, not one? And what about the sun? Let’s pull back the curtain on one of nature’s most familiar mysteries—and discover how Earth, the moon, and the sun perform a slow-motion dance that moves entire oceans.

How the Moon Pulls the Ocean

Any object with mass exerts gravity. That includes you, me, the moon—and the ocean.

Gravity pulls things toward mass. The bigger the mass and the closer you are, the stronger the pull.

The moon is about 1/80th the mass of Earth—and it’s close. Its gravity tugs noticeably on Earth’s oceans.

The water closest to the moon feels a stronger pull than the water on the far side. That difference creates a bulge of ocean on the moon-facing side.

Now imagine Earth spinning beneath that bulge. As your coastline rotates into it, the water rises: high tide. When it rotates away, the water falls: low tide.

High tide happens when your part of the Earth rotates into the ocean bulge pulled by the moon.

But there’s not just one bulge. There’s another—on the opposite side of the planet.

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Why Is There a Bulge on the Far Side Too?

This is the part most explanations skip.

If the moon pulls the water toward it, why does the ocean also bulge away from it?

The Moon Pulls on Everything—Not Just Water

The moon’s gravity pulls on the whole Earth—not just the ocean, but also solid ground. And it pulls unequally:

  • The side facing the moon feels the strongest pull.
  • The far side feels the weakest.
  • The center of Earth is in between.
  • This uneven tug stretches the planet.

But there’s another factor at play: inertia.

A Helpful Analogy: The Car Launch

You’re sitting in a stopped car. The driver floors it. You feel pressed into your seat. That’s inertia—your body resisting acceleration.

Earth feels something similar. As the moon pulls on Earth, our planet is in constant free-fall toward it. That motion creates an equal inertial force across the globe—but the moon’s gravitational pull is not equal.

The result? Tidal force.

Tidal Force = Gravity – Inertia

The tidal force is the difference between:

  • The moon’s varying gravitational pull across Earth
  • The uniform inertial “push” from Earth’s motion

At Earth’s center, the forces cancel out.

  • On the near side, gravity wins → ocean bulges toward the moon
  • On the far side, inertia wins → ocean bulges away

The far-side bulge isn’t caused by the moon pulling the water. It’s caused by the Earth moving away from it.

Two Bulges, Two Tides

As Earth spins, your coastline passes through both bulges. That’s why you get:

  • One high tide when you rotate into the bulge facing the moon
  • Another when you rotate into the far-side bulge

It’s not just a simple pull—it’s a stretch, caused by gravity acting unevenly across a spinning, accelerating planet.

🔗 For the Curious
Explore this tidal force using visual vectors:
👉 PhET Vector Addition Simulation
Deep dive with diagrams and math:
👉 Tidal Force Explained – Fujiwaratko

What About the Sun?

The sun is far away—almost 400 times farther than the moon—but it’s 27 million times more massive. That sheer size gives it significant pull.

The result? The sun contributes about half the tidal force of the moon.

Its gravitational tug creates a second set of tides: solar tides.

Spring Tides: When Forces Combine

Twice a month, the sun, moon, and Earth align—during new and full moons.

Now both gravitational pulls work together, stretching the ocean in the same direction.

  • High tides get higher
  • Low tides get lower

These are called spring tides (not named after the season—they “spring up” in strength).

Neap Tides: When Forces Compete

A week later, the sun and moon form a right angle—during first and third quarter moons.

Now the sun pulls in one direction, the moon in another.

  • High tides are less high
  • Low tides are less low

These milder tides are called neap tides.

It’s not a magical cosmic coincidence that we get extreme tides at full moon.
It’s physics. It couldn’t happen any other way.

Why Some Places Have Big Tides—and Others Don’t

Tides follow a global rhythm—but they don’t look the same everywhere.

Some places see tides rise and fall by meters, like Canada’s Bay of Fundy. Others see only small changes—around 30 centimeters in places like the Gulf of Mexico. And in some seas, like the Mediterranean, tides are barely noticeable.

Geography Matters

Tides are moving waves, not just up-and-down water levels. Their movement depends on space.

  • Wide, shallow bays funnel and amplify tides
  • Narrow straits choke or distort them
  • Deep coastlines often see smaller tides
  • Islands in the open ocean get gentle, regular tides

The shape of the coastline, water depth, and even the slope of the seafloor all play a role.

Why Lakes, Rivers, and Small Seas Don’t Have Big Tides

If the moon pulls on all water, why don’t lakes have tides?

Size and Connection

  • Lakes are too small and enclosed. The gravitational pull is there—but the water can’t move much. Most lake tides are just millimeters.
  • Rivers have a one-way flow. Tidal motion can’t push against that current—except in rare places, like the Amazon, where tidal bores race upstream.
  • Even enclosed seas like the Mediterranean barely experience tides. Narrow connections to the ocean (like the Strait of Gibraltar) limit the flow in and out.

So, Why Did the Water Swallow Your Sunbed?

Because Earth is caught in a cosmic tug-of-war.

The moon pulls most of the strings. The sun adds its strength. Together, they stretch our oceans into two bulges—one toward the moon, one away.

As Earth spins, your shore rotates through those bulges. That’s why you get two high tides each day.

But tides aren’t just about the moon you see in the sky. They’re shaped by invisible forces—and local quirks beneath your feet.

They remind us that even the ordinary shoreline is part of a quiet cosmic dance.

So next time you go to the beach? Maybe set your towel a little farther up.

It’s not magic. It’s physics.

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