Course EEEN 567 — Satellite Engineering • Prepared for 5th Year Undergraduate Electrical Engineering Students. Covers launch vehicles, rocket propulsion, orbital mechanics of ascent, launch operations, and the electrical engineering systems that make a launch possible.
By the end of this study guide, the student should be able to:
A satellite launch is the engineered process of delivering a spacecraft from the surface of the Earth to its intended orbit (or beyond) using a launch vehicle — a rocket whose sole mission ends when the payload is released on the correct trajectory. For an electrical engineering student, launching is where several disciplines converge: control systems steer the vehicle, communication systems maintain the telemetry and command link, power electronics feed the avionics, and signal processing extracts navigation solutions from sensors.
Every orbital launch is fundamentally an energy management problem. To reach a 400 km circular orbit, a vehicle must lift the payload against gravity (potential energy), accelerate it to roughly 7.7 km/s (kinetic energy), and overcome atmospheric drag and steering losses along the way. Because a rocket must also carry its own propellant — and propellant is needed to lift propellant — the required vehicle is far larger than the payload: a typical ratio is that the payload is only 2–4% of the lift-off mass.
Every stage is discarded after burnout. Historically dominant (Ariane 5, Proton, Long March families, PSLV). Simple, reliable, but hardware is lost every flight.
Some or all stages are recovered and reflown. SpaceX Falcon 9 first-stage landings (land or drone ship) and Blue Origin New Shepard are flagship examples. Reuse shifts cost from manufacturing to refurbishment and operations.
| Class | Payload to LEO | Typical vehicles | Typical use |
|---|---|---|---|
| Small-lift | < 2 000 kg | Electron, Vega, LauncherOne | Cubesats, smallsats, dedicated rides |
| Medium-lift | 2 000 – 20 000 kg | Falcon 9, Soyuz-2, PSLV/GSLV | Comms constellations, ISS cargo, science |
| Heavy-lift | 20 000 – 50 000 kg | Falcon Heavy, Ariane 64, Long March 5 | GEO comsats, deep-space probes, modules |
| Super-heavy | > 50 000 kg | SpaceX Starship, NASA SLS, Long March 9 (dev.) | Moon/Mars logistics, mega-constellations |
| Type | Examples | Pros | Cons |
|---|---|---|---|
| Solid | APCP boosters (Ariane SRB, SLS boosters) | Simple, storable, high thrust density, instant readiness | Lower Isp (~260–290 s), cannot throttle or restart |
| Liquid (hypergolic) | MMH/N₂O₄, UDMH/N₂O₄ | Storable, restartable, simple ignition | Toxic; modest Isp (~310–340 s) |
| Liquid (cryogenic) | LOX/LH₂ (Vulcan upper stage, Ariane 6) | Highest Isp (~420–460 s) | Boil-off, complex ground handling, low density |
| Liquid (kerosene) | LOX/RP-1 (Falcon 9, Soyuz) | Good Isp (~300–350 s), dense, flight-proven | Coking, slightly lower performance than H₂ |
Thrust is produced by expelling propellant at high velocity (Newton's third law), plus the pressure thrust at the nozzle exit:
F = thrust (N) • ṁ = propellant mass flow (kg/s) • ve = effective exhaust velocity (m/s) • pe, pa = nozzle exit and ambient pressure (Pa) • Ae = exit area (m²)
Specific impulse, Isp, measures propellant efficiency — thrust per unit weight-flow of propellant:
g₀ = 9.81 m/s² (standard gravity). Higher Isp means more velocity per kilogram of propellant.
The fundamental sizing equation of any launch vehicle relates achievable velocity change to exhaust velocity and the ratio of initial to final mass:
Δv = velocity change (m/s) • m₀ = initial (wet) mass • mf = final (dry + payload) mass • R = mass ratio m₀/mf
Once a stage's tanks are empty, their structure is dead mass. Discarding it (staging) improves the mass ratio of what remains. Optimum staging sizes each stage so that Δv contributions roughly balance structural and propellant fractions. Typical allocations:
| Stage | Typical Δv | Notes |
|---|---|---|
| First stage | 2 – 3.5 km/s | Fights gravity and drag; high thrust, low altitude |
| Second stage | 4 – 5 km/s | Most of the orbital velocity is built here (near-vacuum Isp) |
| Upper / transfer stage | 2 – 3.5 km/s | Perigee/apogee burns, GTO insertion, restart capability |
Total ideal Δv ≈ 9.3 – 10 km/s is required from the vehicle to reach LEO, because roughly 1.5 – 2 km/s is lost to gravity and drag — the ideal (equation) Δv must cover both.
| Component | Fraction of lift-off mass |
|---|---|
| Propellant | ≈ 85 – 90 % |
| Structures & engines | ≈ 6 – 10 % |
| Payload (including adapter) | ≈ 2 – 4 % |
An orbital launch is not a vertical climb — it is a controlled pitch-over that trades altitude for horizontal velocity. A typical profile:
μEarth = 3.986 × 10¹⁴ m³/s² • r = radius from Earth's centre (m). vcirc at 400 km ≈ 7.67 km/s; escape velocity ≈ 10.9 km/s there.
Launching eastward exploits Earth's rotation, providing a free velocity bonus:
| Launch site | Latitude | Rotational bonus (east) |
|---|---|---|
| Equator (e.g., Sea Launch) | 0° | ≈ 465 m/s |
| Kourou (Ariane) | 5.2° N | ≈ 463 m/s |
| Kennedy / Cape Canaveral | 28.5° N | ≈ 409 m/s |
| Baikonur | 45.9° N | ≈ 324 m/s |
| Plesetsk | 62.8° N | ≈ 213 m/s |
The target orbit inclination sets the launch azimuth (for a direct ascent, cos i = cos lat · sin Az, ignoring Earth's rotation). Sites far from the equator cannot reach low inclinations directly, which is why GTO missions favour Kourou.
Geostationary satellites are usually injected into a Geostationary Transfer Orbit (GTO) — a highly elliptical orbit with perigee in LEO and apogee at GEO altitude (35 786 km). An apogee motor (or electric propulsion over months) then circularises at GEO.
r₁ = perigee radius (LEO) • r₂ = apogee radius (GEO = 42 164 km from Earth's centre)
Worked reference (400 km LEO → GEO): Δv₁ ≈ 2.45 km/s, Δv₂ (at apogee) ≈ 1.47 km/s, transfer time ≈ 5.26 hours. Try the calculator in Section 12.
A space launch is a months-long campaign, not just ten minutes of flight. The condensed sequence:
| Site | Country | Latitude | Primary use |
|---|---|---|---|
| Kennedy / Cape Canaveral | USA | 28.5° N | Falcon 9/Heavy, Vulcan, New Glenn |
| Vandenberg | USA | 34.7° N | Polar / SSO launches (Starlink, imaging sats) |
| Kourou (CSG) | French Guiana | 5.2° N | Ariane 6, Vega, Soyuz (historically) |
| Baikonur | Kazakhstan | 45.9° N | Soyuz crewed & cargo, Proton |
| Jiuquan / Xichang / Wenchang | China | ~28° N / 28° N / 19° N | Long March family; Wenchang newest coastal site |
| Satish Dhawan (Sriharikota) | India | 13.7° N | PSLV, LVM3 (Gaganyaan crewed) |
| Guiana / sea platforms / air-launch | Various | — | Mobile concepts move the site to the optimum latitude |
Modern launch vehicles are "flying computer networks with engines attached". The main EE subsystems:
| Subsystem | Function | EE topics involved |
|---|---|---|
| Guidance, Navigation & Control (GNC) | Compute position/velocity/attitude; steer along the reference trajectory; command TVC | State estimation (Kalman filters), digital control, IMU/GPS fusion |
| Flight computers | Run the real-time OS, sequencing, redundancy management | Fault-tolerant computing, triple modular redundancy, voting |
| Telemetry, Tracking & Command (TT&C) | Downlink thousands of channels (pressures, temps, tank levels, bus voltages); uplink commands; ranging | Modulation (PCM/FM, spread spectrum), link budget, antennas |
| Power systems | Batteries + DC/DC converters power avionics; pyro batteries separate for ordnance | Power electronics, battery management, EMC design |
| Pyrotechnics / ordnance | Stage separation, fairing jettison, engine ignition charges | Squib firing circuits, current-limiting, ESD protection |
| Sensors & data acquisition | Pressure transducers, thermocouples/RTDs, accelerometers, rate gyros, valve position | Signal conditioning, ADCs, multiplexing, sampling theory |
| RF & antennas | S-band/C-band telemetry, GPS L-band, FTS receivers, inter-stage links | Antenna theory, link budgets, RFI/EMC compliance |
Launch is the most severe mechanical event in a satellite's life. Structural and electrical designers must qualify the spacecraft against:
| Environment | Typical levels / duration | Design consequence |
|---|---|---|
| Quasi-static acceleration | 3 – 6 g axial, 1 – 2 g lateral (min ~80 s) | Stiff structures; proof-load factor ~1.25 on coupled loads |
| Sinusoidal vibration (liftoff / engine cutoff) | ~0.5 – 1.5 g, 5 – 100 Hz | Qualification by sine sweep on shaker |
| Random vibration (acoustic + engine noise) | ~14 – 17 grms overall, 20 – 2000 Hz, inside fairing | Component mounting, potting, connector locking |
| Acoustic noise | ~140 – 146 dB OASPL near liftoff | Lightweight panel design, acoustic blankets in fairing |
| Shock (separation / pyro events) | Hundreds to thousands of g at source, kHz frequencies | Shock isolation, avoid pyro-sensitive optics nearby |
| Pressure & venting | 0 → vacuum in ~3 min after fairing jettison | Venting paths; prevent "satellite explosion" from trapped air |
| Thermal | Fairing solar soak to cold soak swings | Heaters/blankets; thermal vacuum (TVAC) test |
| EMC | Vehicle transmitters, radar, FTS | EMI hardening; radiated/ conducted susceptibility tests |
Standard verification: workmanship (random vibe + thermal cycle), qualification (1.25× environments, protoflight or dedicated QM model), and acceptance testing of the flight unit. Environmental test standards: SMC-S-016, GSFC-STD-7000, ECSS-E-ST-32.
First-stage recovery and reflight (10+ flights per booster in routine service) reduced marginal launch cost dramatically, enabling rideshare programmes where many smallsats fly as secondary payloads. Electrical engineering highlight: landing uses grid fins (aerodynamic control), throttleable Merlin engines, and real-time GNSS/INS fusion — closed-loop control landing a 25-storey building on a drone ship.
Ariane 5 famously flew two-satellite GTO missions to GEO (dedicated dual launch). Ariane 6 adds a restartable Vinci cryogenic upper stage and a re-ignitable third stage option (A64 vs A62), restoring European autonomous access to space while cutting cost per kg.
Electron (Rocket Lab) pioneered the dedicated smallsat class; LauncherOne (air-launched from a Boeing 747) showed mobile launch concepts. Air launch gives latitude/azimuth freedom and avoids weather scrubs at a fixed pad — at the cost of payload mass.
Use these to check the worked examples and explore "what-if" questions from your tutorials.
Attempt each question, then reveal the answer. Questions are typical of EEEN 567 continuous assessment.
Q1. The Tsiolkovsky rocket equation shows that to double a stage's Δv capability (at fixed Isp), the mass ratio R = m₀/mf must be:
Q2. During ascent, "Max-Q" refers to the point of maximum:
Q3. A launch site on the equator launching due east gains approximately what rotational velocity bonus?
Q4. In the telemetry chain of a launch vehicle, the function of the frame synchronisation word is to:
Q5. GTO (Geostationary Transfer Orbit) insertion requires a perigee-raising burn at apogee of approximately:
Q6. Which electrical subsystem is responsible for destructing the vehicle if it leaves the approved flight corridor?
Q7. Why is the satellite's first longitudinal natural frequency required to be above ~100 Hz when mounted on the launch adapter?
Q8. Cryogenic LOX/LH₂ upper stages are preferred for high-energy orbits mainly because hydrogen offers: