Googolstars Study Guide 8 topics ↓
An interactive astronomy journey · for everyone

One journey,
from Earth to the edge of the universe

Whether you're a curious explorer, a self-taught student, or a teacher looking for inspiration — follow this journey and fly from Earth all the way to the edge of the universe in the Googolstars interactive 3D universe. 8 topics mapped to real cosmic scales, each with key terms, fun Q&A and hands-on mini-activities to learn as you go.

🧑‍🚀 Great for students · self-learners · teachers
Go at your own pace · pause anytime
💰 Completely free
🌐 No signup or install needed
Start exploring the 8 topics Open the 3D universe ↗
How to start

One tool, three steps to get going

No install, no signup. Open the 3D universe and "fly" through every scale yourself by following the topics below — explore on your own, or watch together in class. Either way, it's fun.

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① Open the 3D universe

Launch Googolstars on a computer, tablet or phone and immerse yourself full-screen. You can also project it for the whole class.

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② Fly through the topics

Each topic maps to a scene. Scroll or swipe to zoom out step by step, from Earth to galaxies and superclusters.

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③ Get hands-on and think

Every topic comes with a mini-activity and a thinking question to help concepts stick — try them yourself, discuss with friends, or work in groups in class.

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Bilingual labels

Scenes and terms are available in both English and Chinese, handy for side-by-side learning and for bilingual or cross-disciplinary STEM lessons.

Journey map · near to far

8 topics, one scale line from home to the cosmos

The whole journey is arranged along "cosmic scale" from small to large, so you build an intuitive feel for distance units (kilometres → astronomical units → light-years → megaparsecs) first-hand.

Stop 1
Earth & the Moon
Stop 2
Inner Solar System
Stop 3
Outer Solar System
Stop 4
Edge of the Solar System
Stop 5
Stellar Neighborhood
Stop 6
The Milky Way
Stop 7
Galaxies & Groups
Stop 8
Largest Scales
Topic content · 8 STOPS

A stop-by-stop tour

Each topic stands on its own, but they also read well in order. We suggest following the scale sequence so the feeling of "farther and farther" runs through the whole journey.

Stop 1
Scale: ~380,000 km

Home Base: Earth & the Moon

Home Base · Earth & the Moon
Learning objectives
  • Explain what makes Earth special as the only known planet in the Solar System to host life.
  • Explain how the Moon's gravity causes tides, and why "tidal locking" means we only ever see one side of the Moon.
  • Describe how Earth's magnetic field blocks the solar wind, protects life and creates auroras.
Key terms
Try it yourself

Take a basketball (Earth) and a tennis ball (Moon) and work out how far apart they should be to scale (about 7.5 m), to feel first-hand just how "empty" the space between Earth and Moon is.

Think about it

If Earth had no magnetic field, what threats would life on the surface face? Why do auroras appear mostly near the poles?

Stop 2
Scale: ~a few astronomical units (AU)

The Inner Solar System & the Sun

The Inner Solar System & the Sun
Learning objectives
  • Understand that the Sun is a star that shines through nuclear fusion and is the energy source of the Solar System.
  • Compare the shared features and differences of the four terrestrial planets (Mercury, Venus, Earth, Mars).
  • Introduce the "astronomical unit (AU)" as a scale for describing planetary distances.
Key terms
Try it yourself

Make an "ID card" for each of the four terrestrial planets: diameter, length of a day, whether it has an atmosphere and water. Then rank them by how habitable you think they are, and explain why.

Think about it

Venus and Earth are similar in size — why is one scorching hot and the other suitable for life? Why didn't the asteroid belt merge into a single planet?

Stop 3
Scale: ~30–50 AU

The Outer Solar System & the Kuiper Belt

Outer Solar System & the Kuiper Belt
Learning objectives
  • Distinguish the "gas giants" (Jupiter, Saturn) from the "ice giants" (Uranus, Neptune).
  • Explain the structure of a comet, and why Halley's Comet returns periodically.
  • Learn about the Kuiper Belt and dwarf planets (such as Pluto), and how the definition of "planet" evolved.
Key terms
Try it yourself

Try sorting the eight planets plus Pluto into three groups — "gas / ice / rock" — then think about why Pluto was reclassified as a dwarf planet in 2006.

Think about it

Why did the giant planets all form far from the Sun? Why does a comet's tail always point away from the Sun?

Stop 4
Scale: ~hundreds to 100,000 AU

Edge of the Solar System: Heliosphere & Oort Cloud

Edge of the Solar System · Heliosphere & Oort Cloud
Learning objectives
  • Describe the solar wind and the heliosphere, and understand "how far the Sun's influence reaches."
  • Learn how the Voyager probes became the most distant objects humans have ever sent.
  • Introduce the "light-year" as a distance unit larger than the AU, and learn about the Oort Cloud and long-period comets.
Key terms
Try it yourself

Light travels about 300,000 km per second — work out how long it takes from the Sun to Earth (about 8 minutes), to Neptune, then to the nearest star, to feel first-hand just how big a "light-year" is.

Think about it

What message does the Voyager "Golden Record" carry? If you had to introduce Earth to aliens, what would you include?

Stop 5
Scale: ~tens of light-years

Our Stellar Neighborhood

Our Stellar Neighborhood
Learning objectives
  • Get to know stars beyond the Sun, such as Proxima Centauri, and understand that stars have different colours and temperatures.
  • Explain how spectroscopy and the Doppler effect let us "read" a star's composition and motion (redshift / blueshift).
  • Learn about supernovae and pulsars, and how the explosive death of stars shapes the surrounding space (the Local Bubble).
Key terms
Try it yourself

Recall how an ambulance's pitch changes as it passes (the Doppler effect) and map that onto the redshift / blueshift of starlight; then try ordering stars from "hottest and bluest" to "coolest and reddest" along O→M.

Think about it

Astronomers have never touched a single star — how can they know what elements it is made of? Why are pulsars called "cosmic lighthouses"?

Stop 6
Scale: ~100,000 light-years

Into the Milky Way: Orion Spur & the Galactic Centre

Into the Milky Way · Orion Spur & Galactic Centre
Learning objectives
  • Learn that the Milky Way is a barred spiral galaxy, with the Sun sitting on one of its arms — the Orion Spur.
  • Explain the concept of a black hole, and distinguish stellar black holes from supermassive black holes (Sgr A*).
  • Describe accretion disks and relativistic jets, and understand how a black hole becomes one of the brightest engines in the universe.
Key terms
Try it yourself

Use a stretchy sheet and a heavy ball to see how spacetime is dented into a "gravity well," then roll a small bead around it and think about why not even light can escape a black hole.

Think about it

We live inside the Milky Way — so how can we draw a picture of the whole galaxy? A black hole gives off no light of its own, so how do astronomers "see" it?

Stop 7
Scale: ~millions of light-years

Galaxies & the Local Group

Galaxies & the Local Group
Learning objectives
  • Distinguish different galaxy types, such as spiral, elliptical and irregular galaxies.
  • Learn about the Local Group, with the Milky Way and the Andromeda Galaxy (M31) as its two leading members.
  • Explain how gravitational interactions between galaxies trigger collisions and new rounds of star formation.
Key terms
Try it yourself

Find several galaxy photos and sort them by "shape" to build your own Hubble classification; then predict what will happen when the Milky Way and Andromeda collide in about 4 billion years.

Think about it

When galaxies "collide," the stars almost never actually hit each other — why? What does that tell you about the space inside a galaxy?

Stop 8
Scale: ~520 million light-years to the observable universe

The Largest Scales: Laniakea & the Observable Universe

The Largest Structures · Laniakea & the Observable Universe
Learning objectives
  • Learn about superclusters and the "cosmic web," and how galaxies gather into filaments and voids on the largest scales.
  • Introduce dark matter and dark energy, and the share of the universe's energy each makes up and what it does.
  • Explain that the universe is expanding ever faster, and why the "observable universe" has a boundary. Recap the whole scale journey.
Key terms
Try it yourself

Draw "galaxy" dots on a balloon, blow it up, and watch every dot move away from every other one — that's cosmic expansion and "no centre." Finally, sum up this 8-stop scale journey in a single sentence.

Think about it

Ordinary matter is only about 5% of the universe; the other 95% is dark matter and dark energy — what does that say about "how much we really understand the universe"? Why does the universe have a "visible boundary"?

Tips · GET MORE OUT OF IT

A few ways to go deeper

🎯 Tie it together with "scale"

With each topic, recall which scale the last stop reached, then "zoom out" one more step to gradually build a feel for distance.

🧑‍🚀 Take the controls

Don't just watch — scroll and drag to "fly" yourself. Driving it is far easier to remember than just looking on.

💬 Guess before the reveal

When you reach a "fun Q&A," guess the answer first, then open it to check — it will stick much better.

🔗 Connect across subjects

Notice the links to physics (gravity, light) and maths (ratios, exponents) for a more rounded understanding.

🗣️ Use the "Wiki" button

Every object on a scene page links to Wikipedia — a great starting point for further reading when you want more depth.

🍎 For teachers

Every topic can be projected straight into a lesson; the thinking questions work as class prompts, exit tickets or short writing tasks — use them flexibly.

FAQ

You might be wondering

Is this really free?

Yes. Googolstars and this study guide are free for anyone to use — for self-study, sharing, or quoting and adapting in class — with no signup and no software to install.

What device or connection do I need?

Just a computer, tablet or phone with internet access and a modern browser (Chrome, Edge, Safari, etc.). The 3D content runs smoothly on an ordinary connection.

Do I need a background in astronomy? What level is it for?

No background needed. The content builds up gradually so secondary-school students — or anyone curious — can follow it; if you want to dig deeper, there are physics principles (gravity, spectroscopy, redshift, cosmic expansion) to explore too.

Is it available in other languages?

Yes. Every scene page is available in English, Chinese and other languages. Use the language switcher in the 3D universe, or add a language prefix to the URL — for example /zh-hk for Traditional Chinese.