The Solar System, Grade 8

Every diagram of the solar system is a lie about distance.

The planets get drawn a few centimetres apart because a page cannot hold the truth. Lay the model out on a school field and Neptune is 562 metres from the Sun. That walk is the only way a class ever feels the scale, and it is the one piece of hands-on work this topic offers.

This page covers the Sun and the objects that orbit it: the Sun, the eight planets, dwarf planets, moons, asteroids, comets, meteors, the Kuiper Belt and the shape of the whole system. It does not cover Earth's position and the seasons, light years, the Milky Way, or telescopes. Those are separate units and they get their own page.

Where this fits in the curriculum

Subject Natural Sciences
Grade 8
Term 4
Strand Planet Earth and beyond
Topic The solar system
Status Informal activities. This grade puts all three assessed pieces in Terms 1, 2 and 3, so there is nothing prescribed here
Marks 45 on our worksheet, and the whole sheet is ours

The Sun

A medium-sized star, and the only one close enough to matter to us.

Distance from Earth 150 million km
Light takes 8 minutes 20 seconds
Diameter About 1,4 million km, so about 109 Earths side by side
Mass 333 000 times the mass of Earth
Share of the solar system's mass 99,8 %
Core temperature About 15 million degrees Celsius
Surface temperature About 5 500 degrees Celsius
Age 4,6 billion years, with about 5 billion still to go

Check the light time yourself: 150 000 000 km divided by 300 000 km per second is 500 seconds, and 500 seconds is 8 minutes 20 seconds. That is the same sum our visible light page does from the other direction.

The Sun does not burn

You will see the Sun described as a burning ball of gases, and as having been burning for 4,6 billion years. It is not burning and it never has been.

Burning means combustion, combustion needs oxygen, and there is no oxygen. What the Sun does is fuse hydrogen into helium, turning about 600 million tonnes of hydrogen into helium every second and releasing energy as it goes.

The wrong word does real damage. A learner who thinks the Sun is on fire has no way to answer why it has not run out of air, and no route into understanding what a star actually is.

Sunspots, solar flares and prominences

Feature What it is
Sunspot A cooler, darker patch on the surface, caused by the Sun's magnetic field. Still about 3 500 degrees, so it only looks dark next to 5 500
Solar flare A sudden burst of energy and radiation thrown off the surface
Prominence A loop of glowing gas arching out and back along the magnetic field

Flares reach us. The particles they throw out disturb satellites, radio signals and power grids, and they are what makes the aurora.

Never look at the Sun

Not directly. Not through sunglasses. Not through binoculars, a telescope, a lens, a prism or a pinhole.

Damage to the retina is permanent, and it does not hurt while it is happening, so nothing warns you to stop.

To show sunspots, project the image onto card and stand with your back to the Sun. Never view through anything.

The three tests for a planet

Something is a planet only if all three are true.

  1. It orbits the Sun
  2. It is big enough that its own gravity has pulled it into a round shape
  3. It has cleared its neighbourhood, meaning it is gravitationally dominant in its own orbit

The third one is the one learners leave out, and it is the only one that does any work in the next question.

Why is Pluto not a planet?

Because it passes the first two tests and fails the third.

Pluto orbits the Sun, and it is round. But it sits in the Kuiper Belt among thousands of other icy objects and has not cleared them out of its path. It is one of a crowd rather than the boss of its own orbit.

It was reclassified in 2006 as a dwarf planet, along with Ceres in the asteroid belt and Eris, Haumea and Makemake further out.

Pluto was not demoted for being small. Size is not one of the three tests. What happened in 2006 is that the word "planet" was defined properly for the first time, and Pluto fell on the wrong side of the third test. Pluto did not change. The definition did.

Orbits are ellipses, not circles

You will see a planet defined as travelling in a regular circular path, with the key words repeating "clear circular path". Orbits are ellipses: squashed circles.

Grade 8 does not need the mathematics, but it does need the word, because the consequence is visible. Mars is sometimes about 3 light minutes from us and sometimes about 22. A circular orbit could not do that.

The inner and outer planets

Inner Outer
Which Mercury, Venus, Earth, Mars Jupiter, Saturn, Uranus, Neptune
Made of Rock and metal Mostly hydrogen and helium
Size Small Large
Moons 0, 0, 1, 2 Many
Rings None All four have them. Saturn's are simply the ones you can see

The asteroid belt separates them, and the split exists because of heat. Close to the young Sun it was too hot for ice and gas to hold together, so only rock and metal survived. Further out they could hold together, so the outer planets grew enormous.

A gas giant has no surface. You would sink through thickening gas until it became liquid. Any temperature quoted for Jupiter, Saturn, Uranus or Neptune is a cloud-top temperature, not a surface one, and it is worth saying so rather than letting a learner picture standing on Jupiter.

And Jupiter's temperature is not set by its distance from the Sun alone. Jupiter radiates more energy than it receives, left over from the slow contraction it is still going through.

How many moons does Jupiter have?

Over 90, as counted in 2026. Saturn has over 270.

Planet Moons, counted in 2026
Mercury, Venus 0
Earth 1
Mars 2
Jupiter over 90
Saturn over 270
Uranus at least 28
Neptune at least 16
Pluto 5

You will see Jupiter and Saturn given "just over 60 moons each", and Pluto given three. Pluto has five, and Saturn's count has more than quadrupled.

These numbers move every time a survey finishes, because the new moons are small, dark and a long way off. So write the number with the year next to it. That is what a scientist does, and it is what an examiner should accept.

The part of the answer that never goes out of date: Saturn has the most, Jupiter is second, and the inner planets have almost none.

The asteroid belt

A band of rocky bodies orbiting the Sun between Mars and Jupiter.

It is far emptier than the pictures suggest. Mostly empty space, with rocks a very long way apart. Spacecraft fly through it without difficulty.

Ceres, about 950 km across, is the largest object in it and it is classed as a dwarf planet rather than an asteroid.

One claim to qualify: you will read that asteroids have iron cores just like Earth's. The large ones that melted early did separate into a core and a crust. Most asteroids are rubble and have no core at all.

Meteoroid, meteor and meteorite

Three words for the same rock in three different places.

Word Where it is
Meteoroid Out in space
Meteor Burning up in our atmosphere. The streak of light
Meteorite The piece that survives and reaches the ground

Comets, and which way the tail points

A comet is ice, dust and rock. Close to the Sun the ice turns to gas and it grows a glowing head and a tail.

Part What it is
Nucleus The solid lump of ice and dust
Coma The fuzzy glowing cloud around the nucleus
Tail Gas and dust blown off it

Ask a class which way the tail points before telling them. Almost everyone says it streams out behind, like hair in the wind.

It always points away from the Sun, whether the comet is coming or going, because it is the solar wind and the Sun's own light pushing the gas and dust away. On the way out, a comet travels tail first.

Halley's comet returns every 75 or 76 years. It was last seen from Earth in 1986 and is next due in 2061. A comet loses ice and dust on every close pass, so it cannot keep doing this forever.

The shape of the solar system, and where it ends

Region Where
Inner planets Out as far as Mars
Asteroid belt Between Mars and Jupiter
Outer planets Jupiter out to Neptune
Kuiper Belt Beyond Neptune. Pluto lives here
Oort Cloud Far further out, and a shell rather than a flat belt. Where long-period comets come from

You will see the Kuiper Belt described as being outside the solar system, beyond Neptune. Beyond Neptune is right. Outside the solar system is wrong.

The Kuiper Belt is part of the solar system, and so is the Oort Cloud. The solar system does not stop at Neptune. It goes on as far as the Sun's gravity keeps winning, which is thousands of times further out than Neptune is.

Gravity holds all of it together, and it is the Sun everything orbits because the Sun has 99,8 % of the mass and therefore by far the strongest pull.

The practical: walk the solar system

One period, a field, and a 100 m tape measure. A 5 m tape will not do this.

  1. Cut nine cardboard circles to the model radii in the table below, one per group, and tape each to a stick
  2. Find a straight line about 600 m long. A field boundary, a long driveway, or the pavement down one side of the school
  3. Plant the Sun at one end. Every distance is measured from there
  4. Walk each planet out with the tape and plant it

The scale model table, recomputed

Sizes are at 1 to 1 billion. Distances are at 1 to 8 billion. Those are two different scales, and that matters: see below.

Body Real distance from the Sun Model distance Model radius
Sun 0 m 696 mm
Mercury 58 million km 7,25 m 2,4 mm
Venus 108 million km 13,5 m 6,1 mm
Earth 150 million km 18,75 m 6,4 mm
Mars 228 million km 28,5 m 3,4 mm
Jupiter 778 million km 97,25 m 71,5 mm
Saturn 1 427 million km 178,4 m 60,3 mm
Uranus 2 871 million km 358,9 m 25,6 mm
Neptune 4 498 million km 562,25 m 24,8 mm

Every model distance is the real distance divided by 8 billion. Check any row with a calculator and it comes out.

THE FIGURE THAT IS PRINTED WRONG, AND IT WILL RUIN THE ACTIVITY.

Published versions of this table give Mars a model distance of 26,5 m. At the table's own scale, 228 million km is 28,5 m.

Every other row divides correctly, which is exactly why the error is easy to miss. A class with a tape measure will plant Mars two metres short and nothing on the field will look wrong. Use 28,5 m.

What the class should notice

What they see What it means
All four inner planets fit in the first 30 metres And then there is nothing at all for 70 metres
Jupiter to Neptune takes up most of the walk The outer solar system is mostly emptiness
Earth is a grain 19 metres from a beach ball This is the moment the diagram breaks
Neptune is out of sight of the Sun On most fields you cannot see one from the other. That is the result, not a problem

The honest answer to "is it to scale?"

It is two scales at once, and a class should be told.

The balls are at 1 to 1 billion. The distances are at 1 to 8 billion. So the distances have been squeezed by a factor of eight to make the model fit on a field.

At a single honest scale of 1 to 1 billion:

Body Size Distance from the Sun
The Sun 1,4 m across. A large beach ball
Earth 13 mm. A pea 150 m
Neptune 50 mm 4,5 km

4,5 km is most of the way across a town. That is the real shape of the solar system, and admitting that the field version cheats is more honest and far more memorable than pretending it does not.

If it does not work

Problem Cause Fix
You run out of field 562 m needs a long straight line Halve every distance and tell the class you have, or run it along a pavement
Mars sits wrong next to Earth You used 26,5 m 28,5 m
A group cannot cut its planet out Mercury at 2,4 mm is smaller than a pencil dot Say so. Mark it with a pin head and let the impossibility be the lesson
The class thinks the model is fully to scale Two scales in one table Give them the 4,5 km figure. Then they know what was traded away
The markers blow over Cardboard on sticks Push them in properly, or weight each one with a stone

How the 45 marks are made up

Part Marks
The Sun 10
The planets, inner and outer 10
Dwarf planets, asteroids, comets and meteors 10
Moons, the Kuiper Belt and the shape of it 8
The scale model 7

Nothing in this topic is prescribed for formal assessment. This grade puts all three assessed pieces in Terms 1, 2 and 3. Our worksheet is 45 and the split above is ours.

Free worksheet and marking memo

Both free, no sign up, straight to the PDF.

Related practicals

What you need to run it

The whole practical needs one thing you probably do not already own: a 100 m tape measure at R105. Everything else is cardboard, sticks and a field.

That is the cheapest practical in our whole range, and it produces the one lesson about the solar system that a diagram cannot.

Item Price What it is for
Measuring tape, PVC, 100 m R105 The practical. Buy this one
World globe, 30 cm R400 Earth in the room while you talk about the rest
Solar system wall chart R85 The system at a glance
The planets wall chart R85 Planet by planet
Solar system model, lit R1 700 A demonstration model that shows the orbits turning

One honest note on the wall charts. We hold the astronomy charts in ones and twos, not in depth, and this is the month they sell. If you want a set for a corridor rather than a single chart for a classroom, ask us first and we will tell you what we can actually send this week.

For a learner building a project at home, the solar system model project kit at R68 has the parts in one packet, and it is the one page on our site where the parent and the teacher want different things from the same topic.

The models and charts are in astronomy, and the full chart range is in wall charts.