한국어로 읽기 The Fate of the Stars

All scenes › Chapter 1 Three stars are born

Mass decides fate

The heavier the star, the sooner it dies

View in 3D

Weight decides fate

The three stars have 40, 15 and 1 times the mass of the Sun. Mass is the amount of matter in a star, its weight, in a sense. A heavy star has more fuel, but it uses it up much faster. So the heaviest star dies first. While a Sun-like star lives about 12 billion years, the 40-Sun star is finished in about 5 million years.

Why?To keep from being crushed by its own weight, a heavy star has to keep its center much hotter. That means burning through fuel extremely fast. It has 40 times the mass, but it shines hundreds of thousands of times brighter, so its fuel runs out about 2,400 times sooner.

Learn moreHow a star ends depends roughly on its starting mass. Lighter than about 8 Suns: a white dwarf. Heavier: a supernova explosion and a neutron star. Heavier than about 20 to 25 Suns: a black hole. These limits are rough, because they change with how much mass a star loses and how fast it spins. This documentary follows the real order of deaths, starting with the heaviest star.

When
Heavier dies sooner
Star we are watching
Mass: 40 · 15 · 1 times the Sun
Size · state
Life: about 5 million years · 12 million years · 12 billion years
View this scene in 3D →

Read more

Wikipedia: Stellar evolution · Wikipedia: Mass–luminosity relation

More in the series

Lifetimes and sizes are typical values from models of how stars change (approximate). The black hole horizon size and the teaspoon masses are calculated with official constants. Sizes, distances and speeds in the 3D view are a rough sketch.