Today we are talking about the life — and death — of stars. Low-mass stars live a long time, fusing all their hydrogen into helium over a trillion years. More massive stars like the Sun live shorter lives. They fuse hydrogen into helium, and eventually helium into carbon (and also some oxygen and neon). When this happens they expand, get brighter, and cool off, becoming red giants. They lose most of their mass, exposing their cores, and then cool off over many billions of years.
Chapters:
Introduction: Low Mass Stars 00:00
Hydrogen Fusion 1:21
Life Cycle of Low Mass Stars 2:22
Larger Stars (Like Our Sun) Live Shorter Lives 3:10
Fueled By Fusion 3:58
Red Giants 5:45
White Dwarfs 8:08
The Fate of the Earth 8:59
Review 11:07
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