한국어로 읽기 The Fate of the Stars

All scenes › Chapter 3 A heavy star: supernova and neutron star

Neutron star

A star the size of a city, heavier than the Sun

View in 3D

A star the size of a city

The center left in the middle of the explosion is a neutron star. It is about 1.4 times heavier than the Sun, yet only about 24 km across, about the size of a big city. One teaspoon of it would weigh about 1.9 billion tonnes. It is the densest kind of star in the universe.

Why?When the center collapses, it is squeezed so hard that all the empty space inside its atoms disappears. Electrons are pushed into the atomic nuclei, and almost the whole star is left as particles called neutrons.

Learn moreGravity at the surface of a neutron star is about 130 billion times stronger than on Earth (worked out from average values). The gas scattered by the explosion glows as a cloud for thousands of years. This is called a supernova remnant.

When
About 12 million years old
Star we are watching
Neutron star
Size · state
About 24 km across · 1.4 times the Sun’s mass
View this scene in 3D →

Read more

Wikipedia: Neutron star · Wikipedia: Supernova remnant

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.