Duration of the online course: 3 hours and 31 minutes
New
Build real spaceflight intuition in this free online course—learn orbits, satellites, and rockets, then test your knowledge with quick exercises and a certificate option.
In this free course, learn about
Why rocket science matters in daily life; reliance on satellites (e.g., GPS navigation)
What an orbit is: continuous free-fall around Earth with sufficient sideways speed
Where space begins: the Kármán line and its accepted altitude (~100 km)
Earth orbital regions (LEO/MEO/GEO) and typical uses, incl. GPS in MEO
Kepler’s laws basics; period increases as orbital size (semi-major axis) increases
LEO vs higher orbits: altitude tradeoffs (drag, lifetime, coverage) like ISS vs Hubble
Why GPS uses MEO: wider coverage and stability than LEO with manageable signal strength
Geosynchronous/geostationary conditions and altitude for a 24-hour orbit (~35,786 km)
Polar orbits and why they enable detailed global mapping over repeated Earth rotations
Newton’s laws for spacecraft; why satellites coast in orbit after engines shut off
Why jets can’t reach orbit; rockets work in vacuum and carry oxidizer
Solid vs liquid engines; staging; rocket equation limits on achievable delta‑V
Launch strategy to gain Earth-rotation boost: launch eastward near the equator
Satellite subsystems: structure/bus, power (solar+batteries), comms, imaging, testing
Course Description
Rocket science is not just for engineers. It shows up every time you use GPS, watch a live broadcast, check the weather, or capture a photo that depends on space-based technology. This free online course turns the big ideas behind modern spaceflight into concepts you can actually picture, helping you understand what satellites do, how rockets reach orbit, and why the rules of motion in space feel so different from what we experience on Earth.
You will build a clear mental model of orbits by exploring what it really means for something to be in orbit, where space begins, and how different orbital neighborhoods work. Instead of treating acronyms like LEO, MEO, and GEO as trivia, you will connect each region to practical missions—like why GPS satellites sit where they do, how a spacecraft can seem to hover in the sky, and why certain orbits are ideal for mapping every part of Earth in detail. Along the way, Kepler’s and Newton’s laws become tools you can use to reason about speed, altitude, and orbital periods without needing advanced math.
The course then connects those orbital fundamentals to the physics of launch. You will see why airplanes cannot simply fly to space, why rockets behave the way they do, and what tradeoffs separate solid motors, liquid engines, and advanced propulsion approaches. The logic behind multistage rockets and the rocket equation is explained in an intuitive way, so you can understand why reaching orbital speed is such a demanding challenge and how engineers squeeze the most performance out of a launch. You will also learn why Earth’s rotation matters and how launch direction can influence the energy needed to reach orbit.
Finally, you will step inside a satellite and learn how key subsystems work together: structure, power, communication, imaging, and the harsh testing needed to survive launch and space. Short questions and exercises throughout help you check your understanding and turn interesting facts into durable knowledge. Whether you are exploring astronomy as a hobby or looking to strengthen your science foundation, this course offers a practical, confidence-building path into the world above our atmosphere.
Course content
Video class: 1.1 | Why Rocket Science Matters | Rocket Science for Everyone with Yale’s Marla Geha01m
Exercise: Which everyday activity is used as an example of relying on satellites orbiting about 12,000 miles away?
Video class: 1.2 | What Is an Orbit | Rocket Science for Everyone: How Satellites Orbit with Yale’s Marla Geha05m
Exercise: What best defines an object being in orbit around Earth?
Video class: 1.3 | Where Does Space Begin? | The Karman Line | Rocket Science for Everyone with Yale’s Marla Geha05m
Exercise: What altitude is the internationally accepted boundary where space begins (the Kármán line)?
Video class: 1.4 | Earth’s Orbital Regions | LEO, MEO, GEO in Rocket Science for Everyone with Yale’s Marla Geha03m
Exercise: Which orbital region is defined as 2,000 to 30,000 km above Earth and is where GPS satellites operate?
Video class: 1.5 | Decoding Orbits: Kepler’s Laws08m
Exercise: According to Kepler's third law, what happens to a satellite's orbital period as its orbital distance (semi-major axis) from Earth increases?
Video class: 2.1 | Low Earth Orbit: LEO Satellites13m
Exercise: Why does the Hubble Space Telescope orbit higher than the International Space Station?
Video class: 2.2 | Medium Earth Orbit11m
Exercise: Why are GPS satellites placed in medium Earth orbit (around 20,000 km) rather than low Earth orbit?
Video class: 2.3 | Satellites That Never Move? GEO Orbits | Rocket Science for Everyone with Yale’s Marla Geha09m
Exercise: What condition must be met for a satellite to appear fixed in one spot in the sky?
Video class: 2.4 | LEO, MEO, GEO: Comparing Earth’s Orbits | Rocket Science for Everyone with Yale’s Marla Geha12m
Video class: 2.5 | Mapping the Earth: Polar06m
Exercise: Why are polar orbits especially useful for mapping the entire Earth in detail?
Video class: 2.6 | Orbital Flight: Speed08m
Video class: 2.7 | Deeper Dive: Kepler’s Law16m
Exercise: Approximately how high above Earth’s surface must a geosynchronous satellite orbit to have a 24-hour period?
Video class: 3.1 | Newton's Laws: How Rockets Fly07m
Exercise: Why can a satellite keep moving in orbit even after its engine turns off?
Video class: 3.2 | Why Planes Can’t Reach Space | Rocket Science for Everyone with Yale’s Marla Geha05m
Exercise: Why can’t a satellite use a jet engine to reach orbit?
Video class: 3.3 | Solid11m
Exercise: What is a key advantage of liquid rocket engines compared to solid rocket motors?
Video class: 3.4 | The Rocket Equation: Why 95% Fuel Won’t Cut It | Rocket Science with Yale’s Marla Geha12m
Exercise: According to the rocket equation, which factor most directly limits why a baking soda–vinegar rocket cannot reach orbit?
Video class: 3.5 | Go Further, Faster! Multistage Rockets | Rocket Science for Everyone with Yale's Marla Geha10m
Exercise: What is the main advantage of using multiple rocket stages during launch?
Video class: 3.6 | Unlock Orbital Speed: Launching Rockets | Rocket Science for Everyone with Marla Geha07m
Exercise: To maximize the extra delta V gained from Earth’s rotation when launching to orbit, which launch strategy is best?
Video class: 3.7 | Electric, Nuclear07m
Exercise: Why can electric propulsion (ion rockets) be useful in orbit but not for launching from Earth?
Video class: 4.1 | Understanding Satellite Payloads | Rocket Science for Everyone with Marla Geha04m
Exercise: Which satellite component is the main structural element that holds the satellite’s “guts and brains” together?
Video class: 4.2 | Powering Satellites: Solar Panels05m
Exercise: Why do Earth-orbiting satellites typically use both solar panels and rechargeable batteries?
Video class: 4.3 | How Satellites Talk: Radio Waves | Rocket Science for Everyone with Yale’s Marla Geha08m
Exercise: Why are radio waves commonly used for satellite communication with Earth?
Video class: 4.4 | Hubble to Your Phone: Space Cameras | Rocket Science for Everyone with Yale’s Marla Geha09m
Exercise: What best explains how a digital camera on a satellite forms an image?
Video class: 4.5 | Satellite Survival: Launch07m
Exercise: What is the main purpose of a thermal vacuum chamber test for a satellite?
Video class: 5.1 | Satellite Launches: Sputnik, SWOT09m
Video class: 5.2 | Over and Out: Meet the Team | Rocket Science for Everyone with Yale’s Marla Geha01m
Exercise: Which contribution is credited with creating the animated visualizations used throughout the class?