Lecture 21: Testing Stellar Evolution

Lecture 21: Testing Stellar Evolution

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Lecture 22: The Cosmic Distance Problem

How do we measure distances to astronomical objects that are too far away to use Trigonometric Parallaxes? This first lecture of Unit 4 reviews geometric methods like trigonometric parallaxes, and then introduces the idea of Standard Candles, and how they are used to develop meth ...  Show more

Lecture 23: The Milky Way

What is the Milky Way, and what is our place within it? This lecture introduces the Milky Way, the bright band of light that crosses the sky, and describes how we came to our present understanding of the size and shape of the Milky Way Galaxy, and our location in it. Recorded 200 ...  Show more

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