Free Course Image Descriptive Astronomy: From Orbits to the Big Bang

Free online courseDescriptive Astronomy: From Orbits to the Big Bang

Duration of the online course: 19 hours and 21 minutes

New

Build real astronomy skills in a free online course: explore orbits, stars, galaxies, black holes, and the Big Bang with bite-sized quizzes and learning support.

In this free course, learn about

  • Kepler’s laws: orbital shapes and why planets move faster near perihelion
  • Core observing tools: telescopes, spectroscopy, Doppler shift, and what each reveals
  • How the solar system formed and how mass is distributed among Sun, planets, and debris
  • Inner planet geology/climates, including Venus’s runaway greenhouse effect
  • Outer planets, moons, and small bodies; why meteor showers occur
  • Sun’s structure (photosphere) and energy source: nuclear fusion in the core
  • Stellar properties from spectra and H–R diagram; mass–luminosity relation on main sequence
  • Measuring distances: radar ranging, parallax, standard candles (Type Ia supernovae)
  • Interstellar gas and dust; star and planet formation, including exoplanet detection methods
  • Stellar evolution from birth to death; white dwarf support by electron degeneracy pressure
  • Black holes and relativity: spacetime curvature, event horizon, and evidence for Sgr A*
  • Milky Way structure and how we infer its central supermassive black hole
  • Galaxies, AGN/quasars, Hubble’s law, mergers, and large-scale galaxy evolution
  • Big Bang evidence (CMB) and astrobiology topics including the Fermi paradox

Course Description

If you have ever looked up at the night sky and wondered how astronomers know what they know, this course offers a clear, welcoming path from familiar observations to the biggest ideas in modern science. You will build a descriptive, evidence-based understanding of the universe, learning to connect what we see through telescopes to the physical laws that shape planets, stars, and galaxies.

You will start with motion in the sky and the logic of orbits, developing intuition for how gravity organizes solar systems. From there, you will see how astronomers extract information from faint light using practical methods such as spectroscopy and Doppler shifts, turning color and line patterns into clues about composition, temperature, and motion. Along the way, you will develop confidence reading the kinds of arguments astronomers use, where observations, measurement, and model-building work together.

As you move outward in scale, you will trace the formation and structure of our solar system, compare inner worlds and giant planets, and understand the role of smaller bodies like asteroids and comets. You will also explore our Sun as a representative star, linking what happens at its visible surface to the deeper processes that power it over billions of years. This foundation sets you up to interpret starlight, make sense of stellar lifecycles, and see how clusters and diagrams reveal age and evolution.

The course then expands to dramatic endpoints such as white dwarfs, supernovae, and black holes, clarifying the role of spacetime and extreme gravity without losing sight of the observational evidence behind these ideas. You will step into the structure of the Milky Way, the behavior of galaxies and quasars, and the patterns captured by Hubble’s law. Finally, you will tie it all together with the Big Bang model, the cosmic microwave background, and a thoughtful look at life in the universe and the Fermi paradox. Short exercises throughout help you check understanding and turn big concepts into usable knowledge you can apply to new astronomical questions.

Course content

  • Video class: Introduction and Orbits - Descriptive Astronomy Lecture 51m
  • Exercise: What does Kepler's second law state about a planet's motion in its orbit?
  • Video class: Astronomical Methods - Descriptive Astronomy Lecture 45m
  • Exercise: What can spectroscopy of a distant star tell astronomers?
  • Video class: Formation of the Solar System - Descriptive Astronomy Lecture 36m
  • Exercise: Which statement best describes how mass is distributed in the solar system?
  • Video class: Inner Solar System - Descriptive Astronomy Lecture 46m
  • Exercise: What process is described as the main cause of Venus becoming extremely hot and inhospitable?
  • Video class: Giant Planets, Moons 55m
  • Exercise: Which pair of outer planets are classified as gas giants (rather than ice giants)?
  • Video class: Asteroids, Comets 52m
  • Exercise: What causes a meteor shower?
  • Video class: The Sun: A Garden-Variety Star - Descriptive Astronomy Lecture 47m
  • Exercise: Which layer of the Sun is considered the visible surface that emits most of the Sun’s visible light?
  • Video class: The Sun: A Nuclear Powerhouse - Descriptive Astronomy Lecture 47m
  • Exercise: What process is responsible for powering the Sun’s long-term energy output?
  • Video class: Analyzing Star Light - Descriptive Astronomy Lecture 47m
  • Exercise: What does a star’s Doppler shift in its absorption-line pattern tell astronomers?
  • Video class: A Celestial Census - Descriptive Astronomy Lecture 39m
  • Exercise: What relationship best describes how a main-sequence star’s luminosity depends on its mass?
  • Video class: Celestial Distances - Descriptive Astronomy Lecture 41m
  • Exercise: Which method measures distances by sending radio waves to an object and timing the return signal?
  • Video class: Between the Stars: Gas and Dust in Space - Descriptive Astronomy Lecture 37m
  • Video class: Birth of Stars and Exoplanets – Part 1 - Descriptive Astronomy Lecture 30m
  • Video class: Birth of Stars and Exoplanets – Part 2 - Descriptive Astronomy Lecture 33m
  • Exercise: Which observation method detects an exoplanet by measuring a star’s tiny back-and-forth Doppler shifts caused by the star’s wobble?
  • Video class: Stars from Adolescence to Old Age – Part 1 - Descriptive Astronomy Lecture 26m
  • Video class: Stars from Adolescence to Old Age – Part 2 - Descriptive Astronomy Lecture 34m
  • Exercise: How can astronomers estimate the age of a star cluster using an H–R diagram?
  • Video class: The Death of Stars – Part 1 - Descriptive Astronomy Lecture 40m
  • Exercise: What physically supports a white dwarf against further gravitational collapse?
  • Video class: The Death of Stars – Part 2 - Descriptive Astronomy Lecture 42m
  • Exercise: Why are Type Ia supernovae especially useful for measuring cosmic distances?
  • Video class: Black Holes and Spacetime – Part 1 - Descriptive Astronomy Lecture 50m
  • Exercise: According to general relativity, why does light appear to bend near very massive objects like the Sun?
  • Video class: Black Holes and Spacetime – Part 2 - Descriptive Astronomy Lecture 42m
  • Exercise: What defines the event horizon of a black hole?
  • Video class: The Milky Way – Part 1 - Descriptive Astronomy Lecture 34m
  • Video class: The Milky Way – Part 2 - Descriptive Astronomy Lecture 35m
  • Exercise: Which observation provides strong evidence that Sagittarius A* is a supermassive black hole at the Milky Way’s center?
  • Video class: Galaxies - Descriptive Astronomy Lecture 45m
  • Exercise: What does Hubble’s Law state about distant galaxies?
  • Video class: Quasars, Active Galactic Nuclei, 49m
  • Exercise: What best explains why quasars can appear star-like yet be extraordinarily luminous?
  • Video class: Evolution and Distribution of Galaxies - Descriptive Astronomy Lecture 50m
  • Exercise: What is a key effect of galaxy collisions and mergers on galaxies?
  • Video class: The Big Bang - Descriptive Astronomy Lecture 52m
  • Exercise: What is the cosmic microwave background (CMB) in the Big Bang model?
  • Video class: Life in the Universe - Descriptive Astronomy Lecture 40m
  • Exercise: What is the Fermi paradox concerned with?

This free course includes:

19 hours and 21 minutes of online video course

Digital certificate of course completion (Free)

Exercises to train your knowledge

100% free, from content to certificate

Ready to get started?Download the app and get started today.

Install the app now

to access the course
Icon representing technology and business courses

Over 5,000 free courses

Programming, English, Digital Marketing and much more! Learn whatever you want, for free.

Calendar icon with target representing study planning

Study plan with AI

Our app's Artificial Intelligence can create a study schedule for the course you choose.

Professional icon representing career and business

From zero to professional success

Improve your resume with our free Certificate and then use our Artificial Intelligence to find your dream job.

You can also use the QR Code or the links below.

QR Code - Download Cursa - Online Courses

More free courses at Astronomy

Free Ebook + Audiobooks! Learn by listening or reading!

Download the App now to have access to + 5000 free courses, exercises, certificates and lots of content without paying anything!

  • 100% free online courses from start to finish

    Thousands of online courses in video, ebooks and audiobooks.

  • More than 60 thousand free exercises

    To test your knowledge during online courses

  • Valid free Digital Certificate with QR Code

    Generated directly from your cell phone's photo gallery and sent to your email

Cursa app on the ebook screen, the video course screen and the course exercises screen, plus the course completion certificate