8/10 (Requires grit) Coolness Factor: 10/10 (You learn to speak for the stars)
How does a cloud of hydrogen turn into a main-sequence star, live for billions of years, and die as a white dwarf, neutron star, or black hole? astro 3104
Here is everything you need to know about navigating one of the most rewarding (and mathematically intense) courses in the astrophysics sequence. ASTRO 3104 is typically a third-year undergraduate course designed as the natural successor to introductory astronomy (ASTRO 1xxx/2xxx). While first-year courses focus on descriptions (planets, galaxies, black holes), ASTRO 3104 focuses on derivations . 8/10 (Requires grit) Coolness Factor: 10/10 (You learn
Be warned. You will not survive ASTRO 3104 with memorization alone. The midterm often features a derivation of the Mass-Luminosity Relation ($L \propto M^{3.5}$) from first principles. The midterm often features a derivation of the
For many physics students, the night sky is a canvas of beautiful, static points of light. By the time they enroll in , they know better. This course—often titled "Stellar Astrophysics" or "The Physics of Stars"—is where the gentle twinkle dies and the violent, fascinating physics of nuclear furnaces begins.