Cover image of 14. Stars 1

14. Stars 1

14. Stars 1

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Light Travel Time

Light Travel Time

Transcript: Since light has a finite speed, three hundred thousand kilometers per second, there’s an inevitable conseque... Read more

24 Jul 2011

1min

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White Dwarf Stars

White Dwarf Stars

Transcript: Some stars in the sky, somewhat hotter than the Sun with temperatures of 5 thousand to 10 thousand Kelvin, h... Read more

24 Jul 2011

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Super Giant Stars

Super Giant Stars

Transcript: Certain rare stars in the sky with either red or blue colors are extremely luminous, up to a million times t... Read more

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Giant Stars

Giant Stars

Transcript: A cool main sequence star with a temperature of about three thousand Kelvin lies on the main sequence with a... Read more

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Main Sequence Stars

Main Sequence Stars

Transcript: As was first seen nearly a hundred years ago, when luminosities and effective temperatures are gathered for ... Read more

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HR Diagram and Stellar Size

HR Diagram and Stellar Size

Transcript: The H-R diagram is a plot of spectral class, or equivalently effective temperature, against stellar luminosi... Read more

24 Jul 2011

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Hertzsprung-Russell Diagram

Hertzsprung-Russell Diagram

Transcript: As a way of exploring stellar properties and understanding how stars work, in the early twentieth century tw... Read more

24 Jul 2011

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Stellar Evolution

Stellar Evolution

Transcript: A human lifetime is a blink of an eye compared to the age of the stars which can be hundreds of millions or ... Read more

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Stellar Classification

Stellar Classification

Transcript: Classification is often an important first step towards physical understanding. Imagine you lived in a smal... Read more

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Hydrostatic Equilibrium

Hydrostatic Equilibrium

Transcript: Stars are stable. For most of their lives, fusion provides the energy source. Even though the Sun and othe... Read more

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