The Origins of the Milky Way Galaxy

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The Big Bang left a universe behind that was made of just hydrogen, helium and tiny little sprinkles of lithium. And as it turns out, it's actually quite hard to make stars or any structure from that hot gas. After these very first stars formed and exploded, the heavier elements like carbon, oxygen, magnesium, iron were suddenly present in the gas clouds. That set the stage for everything else to happen, including us here talking today.

Anna Frebel is an astronomer and astrophysicist at MIT. Please support this podcast by checking out our sponsors:
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OUTLINE:
Here’s the timestamps for the episode. On some podcast players you should be able to click the timestamp to jump to that time.
(00:00) – Introduction
(05:26) – First elements
(12:35) – Milky Way
(16:11) – Alien worlds
(19:16) – Protogalaxies
(24:29) – Black holes
(29:27) – Stellar archeology
(38:42) – Oldest stars
(46:32) – Metal-poor stars
(1:02:05) – Neutron capture
(1:07:01) – Neutron stars
(1:12:30) – Dwarf galaxies
(1:17:10) – Star observation
(1:45:27) – James Webb Space Telescope
(1:51:17) – Future of space observation
(1:54:26) – Age of the universe
(2:07:34) – Most beautiful idea in astronomy
(2:11:23) – Advice for young people
(2:20:17) – Meaning of life