How to Build · Class 01

Build a satellite internet network

The physics of Starlink, one measurement at a time

Grade 7 and up4 or 8 weeks90 minutes / weekNo Starlink kit needed

How can a message from a valley with no cable reach a server on another continent in less time than it takes to blink?

A possible message route · follow the reply back, too
  1. Your device
  2. Wi-Fi router
  3. Starlink terminal
  4. Satellite
  5. Ground station
  6. Wider internet & destination

A satellite may relay information to another satellite by laser before reaching a ground station. Radio connects terminals and spacecraft; laser light connects spacecraft to one another. This is a simplified route, not a live network map.

Your mission

Design, build and defend a model network for an island school, a mountain clinic or a ship. Encode a message and measure what reliability costs. Derive the speed your relay needs and calculate how long it stays in view. Close an energy budget across an eclipse. Then break your own design on purpose, measure what happens, and state precisely which claims your evidence supports.

This is an independent enrichment class with no grade-course prerequisites, but it is quantitative throughout. You will need ratio and percentage, substitution into a formula, and a calculator. The Run the numbers section in every lesson is split in two: the core tasks need arithmetic and rearrangement, and the deeper tasks assume Grade 9–12 tools — trigonometry, logarithms and a little Newtonian mechanics. Doing only the core tasks is a complete course.

Choose your course length

One 90-minute session each week. Eight weeks gives time to measure, calculate and redesign; four weeks keeps the same eight lessons and the same physics, with the quantitative work concentrated into fewer, longer blocks.

8 weeks · build, calculate, improve
  1. What a message actually is — Information · binary encoding · error control · systems
  2. Putting information on a wave — Electromagnetic spectrum · modulation · bandwidth · signal-to-noise
  3. Why the relay stays up — Gravitation · circular motion · orbital period · scale
  4. The geometry of being in view — Spherical geometry · elevation angle · footprint · handoff · Doppler
  5. Closing the energy budget — Solar constant · cosine law · energy storage · thermal radiation · propulsion
  6. Where the delay actually comes from — Packet switching · propagation · queuing · throughput · latency budget
  7. Designing under constraint — Link budget · requirements · shared spectrum · orbital debris · tradeoffs
  8. Defending the result — Systems integration · error analysis · reproducibility · bounded claims
4 weeks · the essential mission

Week 1 · Information, and the signal that carries it

15 min: measure a picture in bits and compare parity with triple repetition; 20 min: encode and transmit an 8-bit frame by flashlight over three matched trials; 20 min: change one factor and retest; 20 min: calculate c = fλ for the flashlight and for a 12 GHz downlink; 15 min: apply the Shannon–Hartley ceiling to one channel and explain why the repetition code costs rate.

Lesson 1 + Lesson 2

Week 2 · Orbit, and the geometry of being in view

15 min: derive v = √(GM / r) and evaluate it at 550 km; 15 min: build one consistent scale model and mark both shells; 25 min: run the 12-step visibility model on paper and on screen; 20 min: calculate γ, footprint radius and pass duration at 25° minimum elevation; 15 min: compare slant range at zenith and at the edge, and convert the ratio to decibels.

Lesson 3 + Lesson 4

Week 3 · Power it, then route the message

15 min: size a battery from the solar constant, the eclipse fraction and depth of discharge; 15 min: test the cosine law at three panel angles, or complete the paper budget; 25 min: run the packet model under normal, congested and failed conditions; 20 min: separate propagation, queuing and serialisation in the measured delay; 15 min: compare a fibre route with a vacuum laser relay over the same distance.

Lesson 5 + Lesson 6

Week 4 · Design it, defend it

15 min: write a measurable target with its failure condition; 20 min: build and run a baseline; 20 min: change one variable, retest and record honestly; 15 min: quantify one shared-sky cost — brightness in magnitudes or decay time against altitude; 15 min: demonstrate under a drawn challenge card; 5 min: write the bounded claim your evidence supports.

Lesson 7 + Lesson 8

Eight lessons, one growing project

Session 1 · 90 minutes

What a message actually is

What is the smallest honest unit of a picture, and what does reliability cost?

Information · binary encoding · error control · systemsOpen the lesson →
Session 2 · 90 minutes

Putting information on a wave

What sets the ceiling on how fast a wireless link can carry information?

Electromagnetic spectrum · modulation · bandwidth · signal-to-noiseOpen the lesson →
Session 3 · 90 minutes

Why the relay stays up

What speed does an orbit require, and where does that number come from?

Gravitation · circular motion · orbital period · scaleOpen the lesson →
Session 4 · 90 minutes

The geometry of being in view

How long is a satellite usable, how much ground does it cover, and how many do you need?

Spherical geometry · elevation angle · footprint · handoff · DopplerOpen the lesson →
Session 5 · 90 minutes

Closing the energy budget

Where does the energy come from, where does it go, and how big must the battery be?

Solar constant · cosine law · energy storage · thermal radiation · propulsionOpen the lesson →
Session 6 · 90 minutes

Where the delay actually comes from

What makes a connection feel slow, and why is that not the same as slow?

Packet switching · propagation · queuing · throughput · latency budgetOpen the lesson →
Session 7 · 90 minutes

Designing under constraint

How do you choose between designs when every option costs something measurable?

Link budget · requirements · shared spectrum · orbital debris · tradeoffsOpen the lesson →
Session 8 · 90 minutes

Defending the result

Can someone who was not there reproduce your test and reach your conclusion?

Systems integration · error analysis · reproducibility · bounded claimsOpen the lesson →

What you will learn

  • Measure information in bits, and calculate what an error-detecting or error-correcting code costs in rate.
  • Use c = fλ to place a channel on the electromagnetic spectrum, and explain why bandwidth and signal-to-noise set a hard ceiling on data rate.
  • Derive orbital speed and period from gravity, and show that an orbit is free fall with enough sideways speed.
  • Use the elevation-angle relation cos(ε + γ) = (R / r)·cos ε to calculate a satellite's footprint, pass duration and slant range.
  • Close an energy budget across an eclipse using the solar constant, the cosine law and depth of discharge.
  • Separate propagation delay, queuing delay and throughput, and predict when a vacuum laser relay beats a fibre route.
  • Judge a design against a measurable target under a named failure condition, and state what the measurement cannot support.

Gather your materials

  • Paper or graph paper, pencils, coloured markers and a ruler
  • A scientific calculator, or a phone calculator with sin, cos and log₂
  • A protractor and a length of non-stretch string
  • Reused cardboard, tape and scissors
  • A flashlight, a sheet of opaque card and a stopwatch
  • 20 index cards, 8 counters and a notebook
  • Optional: a rated educational solar-cell kit with a matching load, a multimeter and a lamp

The core class runs on paper, string and a calculator. The solar kit is optional and its lesson has a complete paper pathway. Use scissors with appropriate supervision, keep flashlights out of eyes, and use only correctly rated educational electronics.

How the class works

Each lesson opens with something to try, explains the physics, puts you through a build and a set of matched measurements, then asks you to run the numbers properly — core tasks first, deeper ones after. Every lesson also carries a worked example, a common mistake with its cause, an independent checkpoint and teacher notes. Keep a mission notebook: prediction → method → observations → calculation → evidence → revision.

Classroom models simplify the world, and every lesson says where its own model stops. A result from one is a bounded claim about the model, never a prediction of real service.

Read further

Technical context checked October 20, 2026. The orbital, geometric and energy figures in this class are calculated from published constants and stated assumptions and rounded for teaching; they describe idealised models, not measurements of any operating system. The activities, fictional records and teaching sequence are independently authored, and this class is not affiliated with SpaceX or Starlink.