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

Free astronomy course spanning orbits, the solar system, stars, black holes, galaxies, the Big Bang, and the search for life in the universe.

In this free course, learn about

  • Foundations of Astronomy and Planetary Orbits
  • The Solar System: Planets, Moons, and Small Bodies
  • The Sun and Stellar Light
  • Stellar Properties, Distances, and the Interstellar Medium
  • Star and Planet Formation
  • Stellar Evolution and Stellar Death
  • Black Holes, Relativity, and Spacetime
  • The Milky Way and Other Galaxies
  • Active Galaxies, Cosmic Evolution, and the Big Bang
  • Life in the Universe

Course Description

Descriptive Astronomy: From Orbits to the Big Bang is a free online course for curious minds who want a clear, descriptive tour of the universe, from the motions of nearby worlds to the largest cosmic structures.

Begin with the foundations of skywatching and orbital behavior, then explore how astronomers measure, observe, and infer the properties of distant objects. Travel through the formation of the solar system and get oriented within the inner planets, giant planets, moons, asteroids, and comets.

Move outward to understand the Sun as a typical star and as a powerful engine driven by nuclear processes. Learn how starlight is analyzed to reveal composition, temperature, motion, and distance, and how surveys help map what populates the cosmos.

Discover the interstellar medium of gas and dust, the birth of stars and planetary systems, and the life cycles of stars from youth to old age. Follow stellar evolution to its most dramatic endings, including supernovae and the exotic physics of black holes and spacetime.

Then zoom out to the scale of the Milky Way and other galaxies, including active galactic nuclei and quasars, and see how galaxies evolve and are distributed across the universe. Conclude with an accessible look at Big Bang cosmology and an exploration of the scientific search for life beyond Earth.

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

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