https://wikimd.com/index.php?action=history&feed=atom&title=PulsarPulsar - Revision history2026-04-24T13:41:56ZRevision history for this page on the wikiMediaWiki 1.44.2https://wikimd.com/index.php?title=Pulsar&diff=5647675&oldid=prevPrab: CSV import2024-04-22T07:30:10Z<p>CSV import</p>
<p><b>New page</b></p><div>[[File:PIA18848-PSRB1509-58-ChandraXRay-WiseIR-20141023.jpg|PIA18848-PSRB1509-58-ChandraXRay-WiseIR-20141023|thumb]] [[File:Pulsar_anim.ogv|Pulsar anim.ogv|thumb|left]] [[File:Lightsmall-optimised.gif|Lightsmall-optimised|thumb|left]] [[File:Chart_Showing_Radio_Signal_of_First_Identified_Pulsar.jpg|Chart Showing Radio Signal of First Identified Pulsar|thumb]] [[File:Chandra-crab.jpg|Chandra-crab|thumb]] [[Image:Vela_Pulsar_jet.jpg|Vela Pulsar jet|thumb]] '''Pulsars''' are a type of [[neutron star]], which are highly magnetized, rotating [[star|stellar remnants]] that emit beams of electromagnetic radiation out of their magnetic poles. This radiation can be observed when a beam points towards [[Earth]], appearing as pulses of radiation ranging from radio waves to gamma rays, hence the name "pulsar" - short for pulsating star. The concept of pulsars was first discovered in 1967 by [[Jocelyn Bell Burnell]] and her thesis advisor [[Antony Hewish]], for which Hewish was awarded the [[Nobel Prize in Physics]] in 1974, a decision that was controversial for not recognizing Bell Burnell's contribution.<br />
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== Discovery ==<br />
The first pulsar, known as PSR B1919+21, was discovered by [[Jocelyn Bell Burnell]] and [[Antony Hewish]] in 1967 using a large radio telescope designed to investigate quasars. The signal, initially dubbed "LGM-1" (for "little green men"), was later identified as a rapidly rotating neutron star. This discovery opened a new window in [[astrophysics]], allowing scientists to study the properties of neutron stars and the physics of extremely dense matter.<br />
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== Characteristics ==<br />
Pulsars are characterized by their rapid rotation and strong magnetic fields. Their periods can range from milliseconds to seconds, and they are considered some of the universe's most accurate clocks. The radiation emitted by pulsars is highly directional, and due to their rotation, it sweeps across the sky. When aligned with the Earth, this results in a pulsed signal that can be detected by radio telescopes.<br />
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=== Types of Pulsars ===<br />
There are several types of pulsars, including:<br />
* '''Radio Pulsars''': The most common type, emitting radio waves.<br />
* '''Millisecond Pulsars''': Extremely fast-spinning pulsars with periods of a few milliseconds.<br />
* '''Gamma-ray Pulsars''': Pulsars that emit most of their radiation in the gamma-ray spectrum.<br />
* '''X-ray Pulsars''': These pulsars emit X-rays and are often found in binary star systems.<br />
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== Importance in Science ==<br />
Pulsars have been used as natural laboratories to study the laws of physics under conditions that cannot be replicated on Earth. They have contributed to the understanding of [[general relativity]], [[quantum mechanics]], and the [[equation of state]] of nuclear matter. Pulsars are also used in tests of [[gravitational waves]] and have been proposed as part of a [[galactic positioning system]] for future navigation in space.<br />
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== See Also ==<br />
* [[Neutron Star]]<br />
* [[Black Hole]]<br />
* [[Radio Astronomy]]<br />
* [[Gravitational Waves]]<br />
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[[Category:Astronomy]]<br />
[[Category:Stars]]<br />
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