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astronomy

XTE J1739−285

XTE J1739−285 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 XTE J1739−285 rather than just read about it. In short: XTE J1739−285 is a low-mass X-ray binary in the constellation Ophiuchus, situated approximately 13,000 light-years from Earth. It was first observed on 19 October 1999 by NASA's Rossi X-ray Timing Explorer satellite.

Key takeaways

  • XTE J1739−285 belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect XTE J1739−285 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of XTE J1739−285 from memory before moving on to harder problems.

Reference excerpt

XTE J1739−285 is a low-mass X-ray binary in the constellation Ophiuchus, situated approximately 13,000 light-years from Earth. It was first observed on 19 October 1999 by NASA's Rossi X-ray Timing Explorer satellite. It had previously been claimed that XTE J1739−285 was the fastest-spinning celestial body yet known, with a frequency of 1122 Hz. However, a re-analysis of these data by other astronomers has been unable to reproduce this result. XTE J1739−285 has been proposed as a possible quark star, as well as 3C 58.

References

Worked examples

Example 1 — a first encounter with XTE J1739−285

Start with the simplest possible case. Write down what XTE J1739−285 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 XTE J1739−285 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 XTE J1739−285 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 XTE J1739−285

In research
XTE J1739−285 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 XTE J1739−285 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
XTE J1739−285 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Compact object stubs, Low-mass X-ray binaries, Neutron stars, so understanding it makes those chapters shorter.
In everyday life
Look for XTE J1739−285 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 XTE J1739−285 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what XTE J1739−285 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 XTE J1739−285 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is XTE J1739−285 in simple terms?

XTE J1739−285 is a low-mass X-ray binary in the constellation Ophiuchus, situated approximately 13,000 light-years from Earth. It was first observed on 19 October 1999 by NASA's Rossi X-ray Timing Explorer satellite.

Why does XTE J1739−285 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 XTE J1739−285?

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 XTE J1739−285.

Tags

  • Compact object stubs
  • Low-mass X-ray binaries
  • Neutron stars
  • Ophiuchus

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