A parsec is the distance at which 1 AU subtends an angle of 1 arcsecond. Distance in parsecs is calculated as d = 1/p, where p is parallax in arcseconds.
Duration of the online course: 1 hours and 24 minutes
Boost your physics skills with this free online course in astrophysics and cosmology—stars, distances, and the expanding universe, plus practice questions.
Build a clear, exam-ready understanding of how the universe works, from the life cycle of stars to the evidence for cosmic expansion. This free online course is designed for learners who want to strengthen core physics knowledge in astrophysics and cosmology with explanations that connect key ideas into a coherent picture, rather than leaving you with disconnected facts.
You will explore how stars form when interstellar clouds collapse and what conditions can trigger that process. From there, you will follow stellar evolution through major stages and learn what ultimately determines a star’s final fate. By focusing on the physics behind outcomes such as white dwarfs and what can come after the red giant phase for very massive stars, you’ll gain intuition about how mass, pressure, temperature, and gravity shape a star’s journey.
On the cosmology side, the course helps you become confident with the measurements that allow astronomers to map the universe. You’ll understand how parallax is used to calculate distances, what a parsec actually means, and how the simple relationship between distance and parallax fits into real problem solving. You’ll also connect observational tools like Doppler effects with larger-scale ideas such as Hubble’s Law and the cosmic microwave background, building an evidence-based view of an expanding universe.
Throughout the course, short focused questions and practice-style problems reinforce what you learn so you can apply definitions and equations accurately under exam conditions. By the end, you should be able to explain stellar birth and evolution in physical terms, interpret basic astronomical distance measurements, and describe the observational foundations of modern cosmology with far more confidence.
Explore free online Modern Physics courses and master quantum mechanics, relativity, particle physics, atomic theory, and cosmology at your own pace. Learn through flexible lessons from trusted educators, build career-ready scientific skills, and earn a certificate upon completion. Start studying modern physics online for free today.
Explore free online astrophysics courses and learn about stars, galaxies, black holes, cosmology, space science, and the universe from anywhere. Build valuable astronomy skills at your own pace with expert-led lessons designed for beginners and advanced learners. Enroll today, study for free, and earn a certificate to showcase your knowledge.
Discover free online General Relativity courses with certificates and explore spacetime, gravity, black holes, gravitational waves, Einstein’s field equations, and cosmology. Learn at your own pace through expert-led lessons, build valuable physics skills, and earn a certificate upon completion. Start studying General Relativity online for free today.
1 hours and 24 minutes of online video course
Digital certificate of course completion (Free)
Exercises to train your knowledge
100% free, from content to certificate
What is a parsec, and how is it calculated from parallax?
A parsec is the distance at which 1 AU subtends an angle of 1 arcsecond. Distance in parsecs is calculated as d = 1/p, where p is parallax in arcseconds.
What determines whether a star becomes a white dwarf or undergoes a supernova?
Its initial mass is the key factor. Low- and medium-mass stars shed their outer layers and leave white dwarfs, while very massive stars can explode as supernovae.
How do redshift and Hubble's law provide evidence for an expanding universe?
Light from distant galaxies is redshifted, showing they are moving away. Hubble's law shows that more distant galaxies generally recede faster, supporting cosmic expansion.
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