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Astrophysics - Star Equilibrium

Offered By: Michel van Biezen via YouTube

Tags

Astrophysics Courses

Course Description

Overview

Explore the fundamental concepts of star formation and equilibrium in this comprehensive astrophysics video series. Delve into topics such as nebula collapse, Jeans length, critical mass, hydrostatic equilibrium, and pressure gradients. Learn what triggers a nebula to collapse into a star, understand the significance of Jeans length in stellar formation, and calculate the critical mass required for nebula collapse through practical examples. Gain insights into the principles of hydrostatic equilibrium that govern a star's structure and stability, and examine the role of pressure gradients in maintaining stellar balance. Enhance your understanding of stellar physics and the intricate processes that shape the life cycles of stars.

Syllabus

Astrophysics: Ch. 2 Star Equilibrium (1 of TBD) Playlist Overview
Astrophysics: Ch. 2 Star Equilibrium (2 of TBD) What Makes a Nebula Collapse into a Star?
Astrophysics: Ch. 2 Star Equilibrium (3 of TBD) What is Jeans Length?
Astrophysics: Ch. 2 Star Equilibrium (4 of TBD) What is Critical Mass for Nebula Collapse?
Astrophysics: Ch. 2 Star Equilibrium (5 of TBD) Critical Mass of Nebula Collapse (Example)
Astrophysics: Ch. 2 Star Equilibrium (6 of TBD) Hydrostatic Equilibrium
Astrophysics: Ch. 2 Star Equilibrium (7 of TBD) Pressure Gradient
Astrophysics: Ch. 2 Star Equilibrium (8 of TBD) Pressure Gradient


Taught by

Michel van Biezen

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