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astronomy

XO-2Nb

XO-2Nb 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 XO-2Nb rather than just read about it. In short: XO-2Nb (or rarely XO-2Bb) is an extrasolar planet orbiting the star XO-2N, the fainter component of XO-2 wide binary star in the constellation Lynx. This planet was found by the transit method in 2007 by Burke et al.

XO-2Nb — main illustration
XO-2Nb — illustration

Key takeaways

  • XO-2Nb belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect XO-2Nb to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of XO-2Nb from memory before moving on to harder problems.

Reference excerpt

XO-2Nb (or rarely XO-2Bb) is an extrasolar planet orbiting the star XO-2N, the fainter component of XO-2 wide binary star in the constellation Lynx. This planet was found by the transit method in 2007 by Burke et al. This was the second such planet found by the XO telescope.

Like most planets found by the transit method, it is a roughly Jupiter sized planet that orbits very close to its host star; in this case, it has a surface temperature of about 1200 K, so it belongs to a group of exoplanets known as hot Jupiters. The planet takes 2.6 days to orbit the star at the average distance of 0.0369 AU. The planet has mass of 57% of Jupiter and radius of 97% of Jupiter. The radius is relatively large for its mass, probably due to its intense heating from its nearby star that bloats the planet's atmosphere. The large radius for its mass gives a low density of 820 kg/m3.

See also XO Telescope

References

External links Media related to XO-2b at Wikimedia Commons

Illustrations

XO-2Nb illustration
XO-2Nb: The radial velocity of XO-2 over time, caused by the presence of XO-2 b.
The radial velocity of XO-2 over time, caused by the presence of XO-2 b.

Worked examples

Example 1 — a first encounter with XO-2Nb

Start with the simplest possible case. Write down what XO-2Nb 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 XO-2Nb 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 XO-2Nb 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 XO-2Nb

In research
XO-2Nb 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 XO-2Nb 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
XO-2Nb is common in secondary-school and first-year university syllabi. It links to neighbouring topics Exoplanets discovered in 2007, Giant planets, Hot Jupiters, so understanding it makes those chapters shorter.
In everyday life
Look for XO-2Nb 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 XO-2Nb in 20 minutes

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

Frequently asked questions

What is XO-2Nb in simple terms?

XO-2Nb (or rarely XO-2Bb) is an extrasolar planet orbiting the star XO-2N, the fainter component of XO-2 wide binary star in the constellation Lynx. This planet was found by the transit method in 2007 by Burke et al.

Why does XO-2Nb 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 XO-2Nb?

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 XO-2Nb.

Tags

  • Exoplanets discovered in 2007
  • Giant planets
  • Hot Jupiters
  • Lynx (constellation)
  • Transiting exoplanets

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