Fill the harbour
A day of tides
Fill the harbour
Slide the clock through a day. When do the boats float?
Step through a day. How long from low tide to high tide?
Slide the clock. When do the boats float?
Your turn
Each lab is one step from the video. Change things and see what happens.
Each lab isolates one part of the story. The models are simplified to show the idea.
Slide the sliders and tap the buttons.
Slide the clock through a day. When do the boats float?
Step through a day. How long from low tide to high tide?
Slide the clock. When do the boats float?
Drag the Moon closer or farther. What happens to the stretch?
Halve the distance. Does the stretch double, or grow much more?
Arrows are not to scale: the leftover (tidal) part is drawn much bigger than it really is.
Drag the Moon around Earth. Where are the two bulges?
Drag the Moon. Where is the water lowest?
Slide the Moon around. Watch the two humps follow!
Bulges are drawn far bigger than real: islands far out in the ocean usually see tides of about a metre or less.
Drag Earth or slide the hours. How many high tides does the town get in a day?
Follow the town for two days. How far apart are the high tides?
Slide the time. When is it high tide?
Drag the Moon. Where are the tides biggest? Smallest? Try turning the Sun off.
Find the spring and neap positions. What does the Sun add?
Pick a coast. How many high tides does it get a day?
Compare semidiurnal, mixed and diurnal coasts.
Curve shapes are illustrative. Check a local tide table for real times.
Go to a harbour in the morning. The boats sit on the mud! Come back later. Now the sea is high, and the boats float.
The Moon pulls on the Earth. That pull is called gravity. It pulls hardest on the side near it, and less on the far side. So the Earth gets stretched, just a little.
Rock does not stretch much. But water slides easily. So the sea makes two big humps. One faces the Moon. One is on the other side!
The Earth spins around once a day. When your beach goes through a hump, the sea comes up: high tide. Between the humps, the sea goes down: low tide. On most beaches, that happens two times a day.
Tides are very long waves that make the sea rise and fall over several hours.
Tides are caused mainly by the Moon's gravity, with help from the Sun, and by Earth's spin.17 The Moon pulls hardest on the side of Earth facing it and most weakly on the far side. That difference stretches our planet, and the oceans (which move far more easily than rock) pile up into two bulges: one facing the Moon and one on the opposite side.45 As Earth turns, a coast passes through both bulges, so most coasts get two high tides and two low tides about every 24 hours and 50 minutes.1
Scientists call this stretching the tidal force. Isaac Newton first explained tides this way in 1687.1
Gravity gets weaker with distance: the closer two objects are, the stronger the pull between them. So the pull on the near side of Earth is noticeably stronger than the pull on Earth's centre, and the pull on the far side is weaker still.14
What matters for tides isn't the Moon's pull itself but the difference between the pull at each spot and the average pull on the whole Earth. NASA's Space Place team puts it as a simple subtraction:4
tidal force = Moon's pull at a spot − Moon's average pull on Earth
Do that subtraction all around the globe and you get a stretch: on the near side the leftover points toward the Moon, and on the far side it points away. Along the "waist" of Earth the leftover gently squeezes inward. That's the pattern the toy in chapter 2 shows.
The same trick explains why the Moon beats the Sun at making tides. The Sun pulls on Earth far harder overall (about 177 times harder than the Moon does), but it is so far away that its pull is almost the same on both sides of Earth. The tidal force falls off with the cube of distance, not the square, so distance matters more than mass.1
Because there are two bulges, and Earth spins through both of them. NOAA describes the ocean as shaped like a football pointing at the Moon: the pointed ends are high tide and the flat sides are low tide.3
The near bulge forms because the Moon's pull is strongest there. The far bulge forms because the pull there is weakest: the rest of Earth is pulled toward the Moon a little more than the far-side water is, so that water is "left behind". NOAA explains the far bulge as inertia winning over the Moon's weaker gravity.13
The water doesn't mostly lift straight up. NASA compares it to a puddle on a table: it's much easier to slide water sideways than to lift it. The tide-producing force nudges water sideways across the ocean, heaping it into the two bulges and drawing it away from the regions in between.57
The Moon travels around Earth in the same direction that Earth spins. So after one full turn (24 hours), Earth has to keep turning for about 50 more minutes to face the Moon again. That makes a lunar day (or tidal day) 24 hours and 50 minutes long.13
| Timing | Typical value |
|---|---|
| One lunar (tidal) day | 24 h 50 min |
| High tide to the next high tide | 12 h 25 min |
| High tide to low tide | about 6 h 12 min |
| Shift in tide times from one day to the next | about 50 min later |
| Spring tide to neap tide | about 7 days |
Values from NOAA's tides tutorial; real coasts vary.12 The bulges also don't sit exactly under the Moon; NASA notes they run a little ahead of it, which is one reason you can't read the tide just by looking at the Moon.5
The Sun makes tides too, in exactly the same way, just smaller. The Sun has about 27 million times the Moon's mass, but it is about 390 times farther away, so its tide-making force is only about half the Moon's.15 The solar tide doesn't show up as a separate set of tides. Instead it makes the Moon's tides bigger or smaller.1
Each lunar month brings two spring tides and two neap tides.1 And despite the name, spring tides have nothing to do with the season: the word comes from the tide "springing forth", and they happen all year round.2
| Spring tide | Neap tide | |
|---|---|---|
| Moon phase | New or full | First or third quarter |
| Sun and Moon | In a line with Earth | At a right angle |
| Their stretches | Add together | Partly cancel |
| Tidal range | Largest | Smallest |
| How often | Twice a month | Twice a month |
The Moon's orbit is an oval, so its distance from Earth changes by about 31,000 miles over a month. When it is closest (perigee), tides are bigger than usual.1 When a spring tide lines up with perigee, NOAA calls it a perigean spring tide; the popular name is king tide. This happens 6 to 8 times a year, and those high tides can be more than a foot higher than spring tides when the Moon is far away.6 Tides are also a little larger around early January, when Earth is closest to the Sun.1
If Earth were a smooth ball covered in water, every place would get two equal high tides a day. But continents block the bulges from sweeping around the world, so the water in each ocean basin sloshes in its own complex pattern.1 In the middle of these patterns there are places where the tide hardly rises or falls at all, and the high tide travels around them.9 NOAA groups the results into three types:1
| Type | What happens | Example |
|---|---|---|
| Semidiurnal | Two high and two low tides a day, about equal | Most of the US East Coast |
| Mixed semidiurnal | Two highs and two lows, but of different heights | US West Coast |
| Diurnal | One high and one low tide a day | Parts of the Gulf of Mexico |
The tidal range is the height difference between high and low tide.1 It depends hugely on the shape of the coast. Islands far out in the ocean, away from continental edges, often get tides of 1 metre or less.1 But when the tide runs onto a wide, shallow shelf or into a funnel-shaped bay, it gets squeezed higher.19
Weather matters too. Strong offshore winds push water away and make low tides lower; onshore winds pile water up. Low-pressure storms can bring tides much higher than predicted.14
Every body of water feels the tidal force, but some barely show it. In the Mediterranean, Black and Baltic seas the tidal range is only a matter of centimetres.9 The Great Lakes do have true tides, but even their spring tides are less than 2 inches (5 cm), hidden by changes from wind and air pressure, so NOAA treats them as non-tidal.6
Nowhere far. It hasn't disappeared: it has moved across the ocean toward wherever high tide is happening right now.10 The incoming (rising) tide is called the flood and the outgoing (falling) tide the ebb. The sideways flow is a tidal current, and the quiet pause between them is slack water.1
Tides don't only move the oceans. The Moon stretches the solid Earth too, very slightly, into a football shape. It's far too small to feel, but scientific instruments can measure it.54 Earth returns the favour: its gravity raises tides on the Moon's surface of about 4 to 6 inches (10 to 15 cm).5
For people, tides matter every day: for ships entering harbours, for building bridges and docks, and for fishing, boating and surfing.7 For sea life, the daily rise and fall shapes whole habitats; animals in rock pools and on shores have special ways of surviving being covered and uncovered.11 And because the Moon and Sun move so predictably, tides can be forecast years ahead. Forecasters combine many repeating patterns, often around 40 for a single place, measured from years of observations.910
Want more? See how the Moon changes shape, how gravity works, and why the wind makes waves (tides are waves too, just very long ones).
The Moon's gravity. It pulls harder on the side of Earth facing it than on the far side, which stretches the oceans into two bulges. As Earth spins, coasts move through those bulges and get high tides. The Sun adds a smaller effect, about half as strong as the Moon's.
There are two bulges of water: one facing the Moon and one on the opposite side of Earth. Earth turns through both of them every lunar day (24 hours 50 minutes), so most coasts get two high tides about 12 hours 25 minutes apart.
It doesn't disappear. The water moves across the ocean toward the places that are having high tide. Low tide at your beach means the water is heaped up in a bulge somewhere else.
Every sea feels the tidal force, but some barely show it. The Mediterranean, Black and Baltic seas have tides of only centimetres, and the Great Lakes have true tides of less than 5 cm, so they are treated as non-tidal.
Spring tides happen at new and full Moon, when the Sun, Earth and Moon line up and their tidal effects (stretches) add together: higher highs and lower lows. Neap tides happen at first and third quarter Moon, when the Sun and Moon are at right angles and partly cancel: gentler tides. Each happens twice a month.
The Moon moves along its orbit in the same direction Earth spins. After one full turn, Earth needs about 50 more minutes to face the Moon again, so a lunar day is 24 hours 50 minutes and the tides slide later each day.
"King tide" is a popular name for a perigean spring tide: a spring tide that happens when the Moon is at its closest to Earth. NOAA says these happen 6 to 8 times a year and can push high tides noticeably higher than usual.