In this, the final lecture of the semester, I attempt to review the main, salient points of the course. Whew! Quite a whirlwind!

In this, the LAST lecture of the semester, we discuss General Relativity and Black Holes.

In this lecture we discuss the final stages of the evolution of low and high mass stars. We also learn about Nova and Supernovae. Finally we talk about Neutron stars and begin a discussion on Black Holes

In this lecture we discuss how a low mass star evolves off the main sequence when it runs out of hydrogen to fuse in its core. We follow its evolution from the Main Sequence to a Red Giant to a Supergiant to a Planetary Nebula to a White Dwarf.

In this lecture we discuss the formation of planets and the discoveries of exoplanets around other stars.

In this lecture we continue to discuss the process of star formation from the fragmentation of a giant molecular cloud, to the collapse of the fragment and the formation of the protostar and disk. We also show where the protostar appears on the HR diagram, and how it evolves onto the main sequence.

In this lecture we discuss the hydrogen spin flip transition that produces radiation at 21cm. We also describe the rich and complex molecular chemistry that exists in "molecular clouds", and how these clouds are intimately related to the formation of stars.

In this class we discuss binary stars and how they are used to determine stellar mass. We then begin to discuss the Interstellar Medium.

In this lecture we discuss the basic properties of stars and the stellar Classification system (OBAFGKM) as well as luminosity classes (I through V). We also investigate the the HR diagram and what it infers about stellar properties.

The camera cut out again but we got 40 minutes of discussion on the properties of the Sun and the process of nuclear fusion.