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PSR B1919+21

PSR B1919+21 is a astronomy topic covered in the lgStudy science library. This page brings together a partial reference excerpt, illustrations, worked examples, real-world applications and a short study plan, so you can understand PSR B1919+21 rather than just read about it. In short: PSR B1919+21 is a pulsar with a period of 1.3373 seconds and a pulse width of 0.04 seconds. Discovered by Jocelyn Bell Burnell on 28 November 1967, it is the first-discovered radio pulsar.

PSR B1919+21 — main illustration
PSR B1919+21 — illustration

Key takeaways

  • PSR B1919+21 belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect PSR B1919+21 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of PSR B1919+21 from memory before moving on to harder problems.

Reference excerpt

PSR B1919+21 is a pulsar with a period of 1.3373 seconds and a pulse width of 0.04 seconds. Discovered by Jocelyn Bell Burnell on 28 November 1967, it is the first-discovered radio pulsar. The power and regularity of its signal were briefly thought to resemble an extraterrestrial beacon, leading the source to be nicknamed LGM, later LGM-1 (for "little green men"). The original designation of this pulsar was CP 1919, which stands for Cambridge Pulsar at RA 19h 19m . It is also known as PSR J1921+2153 and is located in the constellation of Vulpecula.

Discovery In 1967, a radio signal was detected using the Interplanetary Scintillation Array of the Mullard Radio Astronomy Observatory in Cambridge, UK, by Jocelyn Bell Burnell. The signal had a 1.337302088331-second period (in 1991) and 0.04-second pulsewidth. It originated at celestial coordinates 19h 19m right ascension, +21° declination. It was detected by individual observation of miles of graphical data traces. Due to its almost perfect regularity, it was at first assumed to be spurious noise, but this hypothesis was promptly discarded. The discoverers jokingly named it little green men 1 (LGM-1), considering that it may have originated from an extraterrestrial civilisation, but Bell Burnell soon cast doubt extraterrestrial life as a source after discovering a similar signal from another part of the sky. The original signal turned out to be radio emissions from the pulsar CP 1919, and was the first one recognised as such. Bell Burnell noted that other scientists could have discovered pulsars before her, but their observations were either ignored or disregarded. Researchers Thomas Gold and Fred Hoyle identified this astronomical object as a rapidly rotating neutron star immediately upon their announcement. Before the nature of the signal was determined, the researchers, Bell Burnell and her PhD supervisor Antony Hewish, considered the possibility of extraterrestrial life:

We did not really believe that we had picked up signals from another civilization, but obviously the idea had crossed our minds and we had no proof that it was an entirely natural radio emission. It is an interesting problem—if one thinks one may have detected life elsewhere in the universe[,] how does one announce the results responsibly? Who does one tell first?

Nobel Prize controversy When Antony Hewish and Martin Ryle received the Nobel Prize in physics in 1974 for their work in radio astronomy and pulsars, Fred Hoyle, Hewish's fellow astronomer, argued that Jocelyn Bell Burnell should have been a co-recipient of the prize. In 2018, Bell won the $3 million Breakthrough Prize in Fundamental Physics for her work.

Cultural references The English post-punk band Joy Division used an image of CP 1919's radio pulses, created by radio astronomer Harold Craft, on the cover of their 1979 debut album, Unknown Pleasures. German-born British composer Max Richter wrote a piece inspired by the discovery of CP1919 titled Journey (CP1919). The English indie rock band Arctic Monkeys used a sound based on the pulses in their music video for "Four Out of Five".

See also Variable star

References

Further reading Hewish, A.; Bell, S. J.; Pilkington, J. D. H.; Scott, P. F.; Collins, R. A. (24 February 1968). "Observation of a Rapidly Pulsating Radio Source". Nature. 217 (5130): 709–713. Bibcode:1968Natur.217..709H. doi:10.1038/217709a0. S2CID 4277613. "K3PGP Experimenter's Corner – Pulsars (List of pulsars for amateur radio astronomers)". K3PGP.org. Archived from the original on 2012-02-10. Retrieved 2008-02-25. "Pulsar Astrometry with the VLBA (Study of Pulsar Parallax, PSR B1919+21 is one of the pulsars studied)". Cornell University. 2004-01-21.

External links Bell, Jon (1996-12-19). "A Tutorial on Radio Pulsars: The discovery of pulsars". Archived from the original on 2012-09-03. Retrieved 2013-06-28. Manchester, R. N.; Hobbs, G.; Khoo, J. "Recording of the first-discovered pulsar CP1919 (PSR B1919+21) made at the Parkes radio telescope in April 2012". CSIRO Astronomy & Space Science: Pulsar Group. Archived from the original on 2016-03-10. Retrieved 2013-06-30.

Illustrations

PSR B1919+21 illustration

Worked examples

Example 1 — a first encounter with PSR B1919+21

Start with the simplest possible case. Write down what PSR B1919+21 claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In astronomy, the smallest case is usually a single object, a single equation or a single measurement. Check that every symbol or term in your sentence has a meaning in that case.

Example 2 — changing one variable

Take the situation from Example 1 and change exactly one quantity: double it, halve it, or set it to zero. Predict what should happen to PSR B1919+21 before you calculate. Comparing your prediction with the result is the fastest way to find out whether you understand the idea or only the words.

Example 3 — an exam-style question

Typical questions about PSR B1919+21 ask you to (a) state it precisely, (b) apply it to given data, and (c) explain a limitation. Practise writing all three answers in under five minutes; the third part is what separates a full-mark answer from an average one.

Applications of PSR B1919+21

In research
PSR B1919+21 appears in astronomy research whenever the underlying quantities have to be modelled precisely. Papers usually cite it as a starting assumption and then explore where it breaks down.
In technology and industry
Engineering practice reuses PSR B1919+21 in design rules, simulations and safety margins. Knowing the idea lets you read a specification sheet and understand why the numbers look the way they do.
In the classroom
PSR B1919+21 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Astronomical objects discovered in 1967, Rotation-powered pulsars, Search for extraterrestrial intelligence, so understanding it makes those chapters shorter.
In everyday life
Look for PSR B1919+21 outside the textbook — in sport, cooking, traffic, electronics or the sky above you. An example you found yourself is remembered far longer than one you were given.

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How to study PSR B1919+21 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what PSR B1919+21 means in your own words.
  3. Compare your version with the excerpt and mark what you missed.
  4. Work through the three examples above with pen and paper.
  5. Explain PSR B1919+21 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is PSR B1919+21 in simple terms?

PSR B1919+21 is a pulsar with a period of 1.3373 seconds and a pulse width of 0.04 seconds. Discovered by Jocelyn Bell Burnell on 28 November 1967, it is the first-discovered radio pulsar.

Why does PSR B1919+21 matter?

Because it connects several astronomy ideas at once: it gives you a definition you can apply, a quantity you can calculate, and a way to check whether a result is plausible.

How should I study PSR B1919+21?

Read the excerpt, restate it from memory, then work through the examples and applications listed on this page. The five-step study plan above takes about twenty minutes.

What does this page cover?

It gives you a compact reference excerpt plus original lgStudy explanations, examples, applications and study material on PSR B1919+21.

Tags

  • Astronomical objects discovered in 1967
  • Rotation-powered pulsars
  • Search for extraterrestrial intelligence
  • Vulpecula

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