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 : History of the Neutron Star

The neutron, an elementary particle with neutral charge in the nucleus of atoms, was predicted by Ernest Rutherford in 1920. Twelve years later, James Chadwick found experimental proof of the existence of neutrons and later received the Nobel Prize for his discovery. Only two years after this discovery, astrophysicists predicted the existence of neutron stars.

In 1934, after months of rigorous calculations regarding star death and of analysis of the properties of neutrons, Fritz Zwicky and Walter Baade published the paper Supernovae and Cosmic Rays. In this paper, they predict, “With all reserve we advance the view that supernovae represent the transitions from ordinary stars into neutron stars, which in their final stages consist of extremely closely packed neutrons.” They believed that these neutron stars were rapidly spinning, dense remnants of dead stars.


Ernest Rutherford


Fritz Zwicky

James Chadwick


Walter Baade