한국어로 읽기 The Fate of the Stars

All scenes › Chapter 2 The heaviest star: a black hole

A black hole is born

A dark hole that not even light escapes

View in 3D

The event horizon

The collapsed center shrinks without end and becomes a black hole. The boundary that not even light can escape is called the event horizon. For a black hole of 15 Suns, this boundary is about 89 km across. Starlight coming from behind the black hole bends around it and looks like a ring.

Why?When gravity is very strong, even the path of light bends. The black hole itself is dark, but light from stars behind it curves around the edge and shows up as a bright ring.

Learn moreThe horizon size comes from a formula in which it grows in step with the mass (using the speed of light and the gravitational constant). The 15-Sun mass is just an example; the real value depends on how much mass the star lost. How a black hole bends time and space continues in the series film “Secrets of Spacetime and Black Holes.”

When
About 5 million years old
Star we are watching
Black hole
Size · state
Horizon about 89 km across (example: 15 Suns)
View this scene in 3D →

Read more

Wikipedia: Black hole · Wikipedia: Event horizon · Wikipedia: Gravitational lens

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.