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astronomy

PSR B1259−63

PSR B1259−63 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 B1259−63 rather than just read about it. In short: PSR B1259−63 is a pulsar and member of an eclipsing binary star system with the blue O9.5Ve-class star SS 2883. The pair has an eccentric orbit that is inclined to the line of sight from Earth by about 36°, leading to a 40-day-long eclipse each time the pulsar passes behind the star.

PSR B1259−63 — main illustration
PSR B1259−63 — illustration

Key takeaways

  • PSR B1259−63 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 B1259−63 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of PSR B1259−63 from memory before moving on to harder problems.

Reference excerpt

PSR B1259−63 is a pulsar and member of an eclipsing binary star system with the blue O9.5Ve-class star SS 2883. The pair has an eccentric orbit that is inclined to the line of sight from Earth by about 36°, leading to a 40-day-long eclipse each time the pulsar passes behind the star. The pulsar has a period of 47.762 milliseconds (ms) and a luminosity of 8.3 × 1035 erg/s. It emits very high energy gamma rays that vary on a time scale of several days. The star SS 2883 has about 22.5 solar masses and is 10.4 solar radii in size. The rate of rotation is about 280 km/s at the equator, or 70% of the breakup velocity.

References

External links http://jumk.de/astronomie/special-stars/psr-b-1259-63.shtml TeVCat 2.0: PSR B1259-63

Illustrations

PSR B1259−63 illustration

Worked examples

Example 1 — a first encounter with PSR B1259−63

Start with the simplest possible case. Write down what PSR B1259−63 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 B1259−63 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 B1259−63 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 B1259−63

In research
PSR B1259−63 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 B1259−63 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 B1259−63 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Centaurus, Compact object stubs, Durchmusterung objects, so understanding it makes those chapters shorter.
In everyday life
Look for PSR B1259−63 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 B1259−63 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what PSR B1259−63 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 B1259−63 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is PSR B1259−63 in simple terms?

PSR B1259−63 is a pulsar and member of an eclipsing binary star system with the blue O9.5Ve-class star SS 2883. The pair has an eccentric orbit that is inclined to the line of sight from Earth by about 36°, leading to a 40-day-long eclipse each time the pulsar passes behind the star.

Why does PSR B1259−63 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 B1259−63?

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 B1259−63.

Tags

  • Centaurus
  • Compact object stubs
  • Durchmusterung objects
  • Eclipsing binaries
  • Emission-line stars
  • High-mass X-ray binaries
  • Millisecond pulsars
  • Multiple star stubs
  • Neutron star X-ray binaries
  • O-type main-sequence stars
  • Variable star stubs

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