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Podcasts de Stars

The Women Astronomers Who Captured the Stars

In the late 19th century, astronomy was a growing field. At the time, Edward Pickering, the...

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Hari Mogosanu: Astrobiologist says that light pollution presents a real risk Newstalk ZB
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Hari Mogosanu: Astrobiologist says that light pollution presents a real risk

The stars in our night sky are vanishing at an alarming rate. New data published in the...

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Percusion FANIA

Hablamos sobre 3 de los percusionistas que pasaron por la legendaria orquesta FANIA. Sus inicios,...

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Black Panther, Early Man, Film Stars Don't Die in Liverpool, and Telephone Torture

Doug Wright and Steve Salles review Black Panther, Early Man, and Film Stars Don't Die in...

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Stars Over Hollywood - Time For Christmas (12-12-53)

Time For Christmas (Aired December 12, 1953) Stars Over Hollywood was a Saturday morning...

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Feos Todos - ECDQEMSD SHOW 3048

HOY: Todos Expulsados - Vacaciones para Todos - Pop Stars - Arroz Quemado - Ella Me Engañó -...

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Cuando sea grande sere YouTube Star

Después de escuchar la entrevista a un Youtube Star me pregunto si me he equivocado de vocación,...

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Fargo, a Farewell and Pop Culture Breadcrumbs?

This week on Pop Culture Happy Hour, NPR Monkey See's Linda Holmes, Stephen Thompson, Glen Weldon...

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Divergent, Hurt Feelings, and a Visit From Jesse Thorn

This week on Pop Culture Happy Hour, NPR Monkey See's Linda Holmes, Stephen Thompson and Glen...

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Cuando sea grande sere YouTube Star

Después de escuchar la entrevista a un Youtube Star me pregunto si me he equivocado de vocación,...

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Lecture 21: Testing Stellar Evolution

What are our observational tests of Stellar Evolution? This lecture discusses how we use...

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Lecture 20: Black Holes

What happens if even Neutron Degeneracy pressure is insufficient to halt the collapse of gravity?...

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Lecture 19: Extreme Stars: White Dwarfs & Neutron Stars

What happens to the cores left behind at the end of a star's life? This lecture introduces these...

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Lecture 18: Supernovae

Once a massive star builds a massive Iron/Nickel core at the end of the Silicon Burning day, it...

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Lecture 17: The Evolution of High-Mass Stars

What happens when a high-mass (more than 4 solar masses) Main Sequence stars runs out of Hydrogen...

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Lecture 16: The Evolution of Low-Mass Stars

What happens to a low-mass star (less than 4 solar masses) when it runs out of core Hydrogen and...

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Lecture 15: The Main Sequence

What are the properties of stars on the Main Sequence? This lecture discusses what happens to a...

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Lecture 14: Star Formation

How do stars form? The Sun is old and in Hydrostatic and Thermal equilibrium. How did it get...

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Lecture 12: As Long as the Sun Shines

How long can the Sun continue to shine, and what source of energy does it tap to keep shining?...

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