Lesson Five Topics

Lesson Five Overview
History of the Neutron Star
The Discovery of the Pulsar
Pulsars and Neutron Stars
How Do Neutron Stars Form?
Properties of Neutron Stars
The Magnetic Field of Neutron Stars
Why Do Neutron Stars Pulse?
Millisecond Pulsars
Pulsar in the Crab Supernova Remnant
Why Study Pulsars?


Activities and Quizzes

Lesson Five : Properties of Neutron Stars

Neutron stars have four basic properties: a small diameter, high density, strong gravity, and strong magnetic field.

Neutron stars are only several kilometers in diameter, often no more than the size of a city. They are at least forty percent more massive than our Sun, however! Consequently, neutron stars are extremely dense, about 1014 (one hundred trillion) times denser than water. A teaspoonful of neutron star could weigh up to one billion tons.

The gravitational force of a neutron star is proportional to its mass and inversely proportional to its radius squared. Thus, neutron stars have very strong gravitational fields. All of the particles in a neutron star are pulled together as tightly as possible, leaving a very smooth, spherical surface. If you tried to visit a neutron star, you would immediately be squished into elementary particles. On the surface of a neutron star, the escape speed (the speed at which you would have to travel in order to escape the gravitational field of a neutron star) is 160,000 km/s, over half the speed of light. Compare this to the escape speed on earth, which is only 11.2 km/s.

Neutron star compared to Manhattan

earthobservatory.nasa.gov