Sky science
Pulsar
Direct answer
Pulsar: A Pulsar is a rotating magnetized neutron star whose sweeping emission beams produce regular detected pulses.
It is a cosmic beacon powered by neutron-star rotation or accretion.
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At a glance
- Found in
- Astronomy & Skywatching
- Related
- Brown Dwarf, Neutron Star, Stellar Black Hole, Supernova
It is a cosmic beacon powered by neutron-star rotation or accretion.
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The story behind Pulsar
Jocelyn Bell Burnell identified the first pulsar signals in 1967.
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Why Pulsar matters
Pulsar’s timing probes gravity, interstellar matter, companions, and gravitational waves.
How to read Pulsar
Correct pulse arrival times for observatory motion and propagation delays.
Pulsar in practice: an example
A millisecond pulsar can rotate hundreds of times each second with exceptional timing stability.
Where readings of Pulsar go wrong
Pulses do not mean the star switches on and off; beam geometry sweeps past Earth.
Sources and editorial method
Research references used for this entry include:
- NASA Science: Stars - NASA overview of stellar birth, main-sequence evolution, giant phases, remnants, and supernovae.
- NASA Science: Universe Glossary - NASA definitions for common stellar, galactic, orbital, and high-energy astronomy terms.
- Source
- The Great Almanac Dictionary
- Category
- Astronomy & Skywatching
- Last updated
- 2026-09-26
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Common questions
What is a Pulsar?
A Pulsar is a rotating magnetized neutron star whose sweeping emission beams produce regular detected pulses.
What do people get wrong about a Pulsar?
Pulses do not mean the star switches on and off; beam geometry sweeps past Earth.
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