Body 101 · Special Lesson · Lesson 14 · Ages 10 to 13

The Solar System and the Universe In Depth

The iron in our blood and the calcium in our bones were once inside the heart of a star. This lesson shows how the Sun shines, why the planets don’t fall into the Sun, why the Moon changes shape every night, how stars are born and die, how many years light takes to reach our eyes, and how scientists know the Universe is about 13.8 billion years old.

The Sun close up, its glowing orange granular surface dotted with sunspots and looping prominences arching off the edge, against deep blue space
1 · The SunA natural nuclear reactor

How does the Sun shine?

The Sun doesn’t burn like a campfire. At its centre, enormous heat and pressure squeeze hydrogen nuclei together until they fuse into helium. A tiny bit of mass goes missing along the way and turns into energy, following Einstein’s most famous equation, E = mc². Tap each layer to see what it does.

How big is it?

To line Earths up across the Sun, you’d need about 109 of them. And if you poured Earths into the Sun, about 1.3 million would fit inside. The Sun holds about 99.86 per cent of all the mass in the Solar System, so all the planets put together are just small crumbs orbiting around it.

How much does it burn each second?

Every second, the Sun turns about 4 million tonnes of mass into energy. That sounds like a lot, but it has so much mass that it can keep going like this for about another 5 billion years. The Sun is about 4.6 billion years old now, right in the middle of its life.

Never look at the SunNever look at the Sun with your bare eyes, through binoculars or a telescope, or through sunglasses, even during an eclipse. Focused sunlight can damage the retina within a few seconds without any pain, and the damage is often permanent. Only ever use proper, certified eclipse glasses.
The eight planets in a row from left to right: Mercury, Venus, Earth, Mars, Jupiter, ringed Saturn, Uranus and Neptune, with the edge of the Sun on the far left
2 · The planetsEight planets and their small neighbours

Meet the planets one by one

The four inner planets are rocky. The four outer planets are giants made mostly of gas and ice. Between the two groups lies the asteroid belt. Tap to choose a planet.

Saturn and its wide rings seen at a slight tilt, the planet’s shadow falling across the rings
Saturn and its ringsThe rings are billions of chunks of ice, from the size of a grain of sand to the size of a house. They stretch hundreds of thousands of kilometres wide but are only about ten metres to one kilometre thick. Shrunk down to the size of a football pitch, they would be thinner than a sheet of paper.
A close-up of Jupiter’s cream, orange and brown cloud bands and the oval Great Red Spot storm
Jupiter’s Great Red SpotA giant storm that has been raging for at least several hundred years, big enough to swallow the whole Earth. Jupiter spins faster than any other planet: one day there lasts less than 10 hours.
Earth and the Moon seen from space, the smaller grey Moon in front of the larger blue and white Earth
Earth and the MoonThe Moon is about a quarter as wide as Earth and about 384,000 kilometres away. That gap is just wide enough to line up all the other planets side by side.

Try it: shrink the Solar System to fit a school field

Imagine the Sun is a ball 30 centimetres wide, placed in the middle of the field. How small would each planet be, and how far away?

Try it: take your scales to other worlds

Your mass stays the same everywhere, but gravity is different, so the scales show a different number. Type in what the scales show on Earth.

kilograms

Why isn’t Pluto a planet any more?

In 2006, astronomers around the world agreed that a planet must pass three tests. One: it orbits the Sun. Two: it is big enough for its own gravity to pull it into a round shape. Three: it has cleared its orbit, meaning it owns its path. Pluto passes the first two, but it orbits among thousands of other icy objects in the Kuiper Belt, so it was classed as a dwarf planet. It’s a great example of science updating its definitions as we learn more.

A satellite with solar panels orbiting above Earth, a golden orbit line curving around the planet over swirling storm clouds and the blue edge of the atmosphere
3 · GravityNewton, Kepler, Einstein

Why don’t the planets fall into the Sun?

In 1687, Isaac Newton explained that everything with mass pulls on everything else. The more mass, the stronger the pull, and if you move twice as far away, the pull drops to a quarter. Planets are actually falling towards the Sun all the time, but they move sideways so fast that they keep missing it. That is what an orbit is. Try firing Newton’s cannon.

Start at 7.9 kilometres per second, then slowly go lower or higher

Why do astronauts float?

The International Space Station is only about 400 kilometres up, where gravity is still about 90 per cent as strong as on the ground. Astronauts float because they and the station are falling together all the time, while shooting sideways at about 28,000 kilometres per hour, so they keep falling around the Earth, just like the cannonball at 7.9 in the simulation.

Kepler’s three laws

PlanetDistance aPeriod T (years)T² ÷ a³

Distance a is measured in astronomical units, where the distance from Earth to the Sun equals 1. Look at the last column: every planet gets almost exactly 1. Kepler found this law from the numbers alone, before Newton could explain why.

Einstein: space can bend

In 1915, Albert Einstein put forward the general theory of relativity. He said gravity isn’t an invisible pulling force: it is mass bending space and time. Picture a bowling ball on a trampoline. A marble rolling past curves towards it because the surface dips, not because a string is pulling it. The theory predicted that starlight would bend as it passed close to the Sun, which was really measured during the 1919 solar eclipse, and it predicted gravitational waves, which were first detected in 2015.

It’s in your phone every day Clocks on GPS satellites run about 38 microseconds a day faster than clocks on the ground, because they are farther from Earth’s gravity and moving fast. If engineers didn’t correct for this using Einstein’s equations, the maps on your phone would drift off by about 10 kilometres every day.
A golden full Moon rising over green rice fields at dusk, with palm trees, a wooden hut and distant mountains
4 · The MoonPhases and eclipses

Why does the Moon change shape every night?

Half of the Moon is always lit by the Sun. What changes is how much of that bright half we can see from here. It is not Earth’s shadow blocking it, a mistake that lots of people, even grown-ups, make. Drag through one whole month, which lasts about 29.5 days.

Sunlight

A total solar eclipse: the black disc of the Moon covering the Sun, wispy white corona streaming around the edge and small pink prominences
Total solar eclipseThis happens when the Moon moves in front of the Sun at new moon. The Sun is about 400 times wider than the Moon, but it is also about 400 times farther away, so they look exactly the same size in the sky. This lucky coincidence lets us see the white corona around the edge.
A total lunar eclipse: a coppery red Moon above a lake and mountains among stars and the Milky Way
Lunar eclipse: a red MoonThis happens on a full moon night, when the Moon moves into Earth’s shadow. But it doesn’t go completely dark, because Earth’s atmosphere bends red light into the shadow. It’s as if every sunrise and sunset on Earth were shining onto the Moon at once. It’s safe to watch with your bare eyes.

Why don’t eclipses happen every month?

The Moon’s orbit is tilted about 5 degrees compared with Earth’s orbit, so most of the time the Moon passes above or below the straight line between Earth and the Sun. Eclipses can only happen when all three line up exactly, which comes round about twice a year.

Always the same face, and slowly drifting away

The Moon spins around once in exactly the time it takes to orbit Earth once, so we always see the same face. The far side isn’t dark: it gets sunlight at new moon. The Moon’s pull causes two high tides a day, and the Moon is slowly moving away from Earth by about 3.8 centimetres a year, about as fast as your fingernails grow.

A star-forming nebula with towering pillars of dust and gas glowing gold and blue, newborn stars shining inside
5 · StarsBorn, living and dying

The life of a star, and how we are made of stars

Every star is born from a cloud of gas and dust collapsing under its own gravity, but how it ends depends on how heavy it was at birth. The heavier the star, the hotter, brighter and shorter-lived it is.

Try it: a star’s colour tells its temperature

5,800 K

Kelvin is the temperature unit scientists use. Zero kelvin is the coldest anything can possibly be. Subtract 273 to get degrees Celsius. Red stars are the coolest and blue-white stars are the hottest, the opposite of the red and blue taps we’re used to.

Try it: stars born with different masses

A huge glowing red giant star beside a tiny yellow Sun-like star on the left for comparison
A red giant compared with a Sun-like starIn about 5 billion years, when the hydrogen in its core runs out, the Sun will swell into a red giant hundreds of times bigger than it is now, and may swallow Mercury and Venus. Betelgeuse in Orion, which you can see during Thailand’s cool season, is a red supergiant like this.
A black hole: a perfectly dark round shadow ringed by glowing light and a swirling disc of orange and golden hot gas bent around it
A black hole and its disc of hot gasA black hole is a region where gravity is so strong that not even light can escape once it crosses the event horizon. We can spot one from the super-hot gas swirling around it. The first real image of a black hole came out in 2019, and an image of the black hole at the centre of our own Milky Way came out in 2022.
We are made of starsThe hydrogen in the water we drink was made in the very early Universe. But the oxygen we breathe, the carbon in every cell, the calcium in our bones and the iron in the haemoglobin that carries oxygen in our blood were all forged inside earlier stars, then blasted out when those stars died. Most heavy elements such as gold come from collisions between neutron stars.
A golden beam of light shooting from the Sun on the left across dark space to a small Earth on the right
6 · Light and distanceLooking far away means looking into the past

A light year is a distance, not a time

Light travels at about 300,000 kilometres per second, fast enough to go round the Earth seven and a half times in one second. The distance light travels in one year is called a light year, about 9.46 trillion kilometres. And because light takes time to travel, whenever we look far away, we are seeing the past. Pick a destination and compare travel times.

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Travelling at the speed of light
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Voyager 1, about 61,000 km per hour
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A car at 100 km per hour, without stopping

The star you see tonight may be a picture from the Ayutthaya period in Thailand

The light from Betelgeuse reaching your eyes tonight set off over 500 years ago, during the Ayutthaya period in Thailand. If it had exploded yesterday, we wouldn’t find out for hundreds of years. And the light from the Andromeda Galaxy, which you can see with your bare eyes in a very dark place, set off about 2.5 million years ago, before our own species of human even existed.

Our home in the Milky Way

The Milky Way is a spiral galaxy about 100,000 light years across, with hundreds of billions of stars. The Sun is about 26,000 light years from the centre, and it takes about 230 million years to go round the centre once. The last time we were at this spot, the very first dinosaurs were just appearing on Earth.

Hundreds of galaxies of many shapes and colours, spirals and ellipticals, scattered across space
7 · The UniverseThe Big Bang theory

How did the Universe begin?

Scientists have found that the Universe is expanding. If you run time backwards, everything must once have been packed together, extremely hot and dense, about 13.8 billion years ago. We call that event the Big Bang, but the name is misleading. It wasn’t an explosion flying out into empty space. It was space itself stretching. Try blowing up a balloon.

Seen from our home galaxy

+0
Nearby galaxy, extra distance
+0
Distant galaxy, extra distance

Every dot moves away from every other dot. No dot is the centre, and the farther dots move away faster. This is what Edwin Hubble saw in the light of real galaxies in 1929.

The balloon isn’t expanding into the room Only the balloon’s surface is the part to compare. The real Universe has no edge to expand past, and there is no outside.

Timeline of the Universe

Three pieces of evidence

What is the Universe made of?

5
27
68

Ordinary matter, which makes up stars, planets and us, is only about 5 per cent. About 27 per cent is dark matter, which we can’t see but which has gravity, and about 68 per cent is dark energy, which makes the Universe expand faster and faster. Nobody knows yet what either of them really is.

A theory is not a guessIn science, a theory is an explanation that has been tested against evidence many times and correctly predicts new things. For example, the Big Bang theory predicted a faint glow across the whole sky before anyone actually found it. But science is also honest enough to say what it doesn’t know yet, such as what came before the Big Bang, or whether the Universe goes on forever.
A white observatory dome open to show its telescope, on a forested mountain top beneath the Milky Way arching across a starry sky
8 · ExploringHumans head into space

How we explore space, and how the body changes

Telescopes carry our eyes billions of light years away, space probes have reached every planet, and people have lived on the space station without a break since 2000. Thailand is taking part too.

The James Webb Space Telescope with its gold hexagonal mirror above a layered silver sunshield, floating among galaxies
The James Webb Space TelescopeIts mirror is 6.5 metres wide, made of 18 gold-coated hexagons. It floats about 1.5 million kilometres from Earth and sees infrared light that our eyes can’t, so it can spot galaxies that formed just a few hundred million years after the Big Bang.
A six-wheeled rover with a mast camera and robotic arm sampling rock on the red rocky ground of Mars under a pinkish-purple sky
Rovers on MarsCar-sized robots drive themselves across the red ground, collecting rock samples to look for signs of past life. Commands from Earth take several minutes to arrive, so the rovers have to make some decisions on their own.

Thailand and space

The National Astronomical Research Institute of Thailand (NARIT) runs the Thai National Observatory on Doi Inthanon, with a telescope whose mirror is 2.4 metres wide. Thailand also has its own Earth-observation satellite, THEOS-2, launched in 2023, which takes pictures to help plan for water, forests and disasters.

Exoplanets

Astronomers have confirmed more than 6,000 planets orbiting other stars. Some sit in a zone that is neither too hot nor too cold, where water could be liquid. This is called the habitable zone. But so far, no evidence of life beyond Earth has been found.

Our bodies in space

That’s why astronauts on the station must exercise for about two hours a day, and space doctors check their bodies throughout the mission. Space medicine is one more career for kids who love both the human body and the stars.

Game: sort the space objects

Read the name and choose what it is. Get answers right in a row for bonus points. You have 45 seconds.

045 seconds
Press to start the game

Review12 questions

Test yourself

Correct: 0 of 12

Fancy a game on this lesson?

Every question from this lesson is in the Body 101 arena. Race the clock, duel someone at home, play as a team, beat the bosses, or practise with no timer at all.