Lecture Description
The class begins with a discussion on transits � important astronomical events that help astronomers to find new planets. The event occurs when a celestial body moves across the face of the star it revolves around and blocks some of its light. By calculating the amount of light that is being obscured astronomers can obtain important information about both star and planet, such as size, density, radial velocity and more. The concept of planetary migration is explained in order to better understand the dramatic differences between bodies in the Inner and Outer Solar System. Finally, potential problems in the Solar System that may occur as a result of migration are addressed.
Course Index
- Introduction
- Planetary Orbits
- Our Solar System and the Pluto Problem
- Discovering Exoplanets: Hot Jupiters
- Planetary Transits
- Microlensing, Astrometry and Other Methods
- Direct Imaging of Exoplanets
- Introduction to Black Holes
- Special and General Relativity
- Tests of Relativity
- Special and General Relativity (cont.)
- Stellar Mass Black Holes
- Stellar Mass Black Holes (cont.)
- Pulsars
- Supermassive Black Holes
- Hubble's Law and the Big Bang
- Hubble's Law and the Big Bang (cont.)
- Hubble's Law and the Big Bang (cont.)
- Omega and the End of the Universe
- Omega and the End of the Universe
- Dark Matter
- Dark Energy and the Accelerating Universe and the Big Rip
- Supernovae
- Other Constraints: The Cosmic Microwave Background
- The Multiverse and Theories of Everything
Course Description
In this course, Yale Prof. Charles Bailyn focuses on three particularly interesting areas of astronomy that are advancing very rapidly: Extra-Solar Planets, Black Holes, and Dark Energy. Particular attention is paid to current projects that promise to improve our understanding significantly over the next few years. The course explores not just what is known, but what is currently not known, and how astronomers are going about trying to find out.
This Yale College course, taught on campus twice per week for 50 minutes, was recorded for Open Yale Courses in Spring 2007.