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SWIFT J1756.9−2508

SWIFT J1756.9−2508 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 SWIFT J1756.9−2508 rather than just read about it. In short: SWIFT J1756.9−2508 is a millisecond pulsar with a rotation frequency of 182 Hz (period of 5.4945 milliseconds). It was discovered in 2007 by the Swift Gamma-Ray Burst Explorer and found to have a companion with a mass between 0.0067 and 0.030 solar masses.

Key takeaways

  • SWIFT J1756.9−2508 belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect SWIFT J1756.9−2508 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of SWIFT J1756.9−2508 from memory before moving on to harder problems.

Reference excerpt

SWIFT J1756.9−2508 is a millisecond pulsar with a rotation frequency of 182 Hz (period of 5.4945 milliseconds). It was discovered in 2007 by the Swift Gamma-Ray Burst Explorer and found to have a companion with a mass between 0.0067 and 0.030 solar masses. It is thought that the companion is the remnant of a former companion star, now stripped down to a planetary-mass core. The pulsar is accreting mass from this companion, resulting in occasional violent outbursts from the accumulated material on the neutron star.

Planetary system SWIFT J1756.9-2508's only known planet is notable for its orbital period of less than an hour, about 54 minutes and 43 seconds.

References

Krimm, H. A.; Markwardt, C. B.; Deloye, C. J.; Romano, P.; et al. (October 2007). "Discovery of the accretion-powered millisecond pulsar SWIFT J1756.9-2508 with a low-mass companion". Astrophysical Journal Letters. 668 (2): L147–L150. arXiv:0709.1693. Bibcode:2007ApJ...668L.147K. doi:10.1086/522959. S2CID 120700539. Krimm, H. A.; Markwardt, C. B.; Deloye, C. J.; Romano, P.; et al. (October 2009). "ERRATUM: Discovery of the accretion-powered millisecond pulsar SWIFT J1756.9-2508 with a low-mass companion". Astrophysical Journal Letters. 703 (2): L183. arXiv:0709.1693. Bibcode:2009ApJ...703L.183K. doi:10.1088/0004-637X/703/2/L183. S2CID 54031388.

External links Universe Today, Pulsar Has Almost Completely Devoured a Star SIMBAD, "SWIFT J1756.9-2508" (accessed 2010-11-06)

Worked examples

Example 1 — a first encounter with SWIFT J1756.9−2508

Start with the simplest possible case. Write down what SWIFT J1756.9−2508 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 SWIFT J1756.9−2508 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 SWIFT J1756.9−2508 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 SWIFT J1756.9−2508

In research
SWIFT J1756.9−2508 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 SWIFT J1756.9−2508 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
SWIFT J1756.9−2508 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Accreting millisecond pulsars, Astronomical objects discovered in 2007, Compact object stubs, so understanding it makes those chapters shorter.
In everyday life
Look for SWIFT J1756.9−2508 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 SWIFT J1756.9−2508 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what SWIFT J1756.9−2508 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 SWIFT J1756.9−2508 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is SWIFT J1756.9−2508 in simple terms?

SWIFT J1756.9−2508 is a millisecond pulsar with a rotation frequency of 182 Hz (period of 5.4945 milliseconds). It was discovered in 2007 by the Swift Gamma-Ray Burst Explorer and found to have a companion with a mass between 0.0067 and 0.030 solar masses.

Why does SWIFT J1756.9−2508 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 SWIFT J1756.9−2508?

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 SWIFT J1756.9−2508.

Tags

  • Accreting millisecond pulsars
  • Astronomical objects discovered in 2007
  • Compact object stubs
  • Exoplanet stubs
  • Hypothetical planetary systems
  • Low-mass X-ray binaries
  • Neutron star X-ray binaries
  • Sagittarius (constellation)
  • Variable star stubs

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