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astronomy

OH/IR star

OH/IR star 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 OH/IR star rather than just read about it. In short: An OH/IR star is an asymptotic giant branch (AGB), a red supergiant (RSG), or a red hypergiant (RHG) star that shows strong OH maser emission and is unusually bright at near-infrared wavelengths. In the very late stages of AGB evolution, a star develops a super-wind with extreme mass loss.

OH/IR star — main illustration
OH/IR star — illustration

Key takeaways

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

Reference excerpt

An OH/IR star is an asymptotic giant branch (AGB), a red supergiant (RSG), or a red hypergiant (RHG) star that shows strong OH maser emission and is unusually bright at near-infrared wavelengths. In the very late stages of AGB evolution, a star develops a super-wind with extreme mass loss. The gas in the stellar wind condenses as it cools away from the star, forming molecules such as water (H2O) and silicon monoxide (SiO). This can form grains of dust, mostly silicates, which obscure the star at shorter wavelengths, leading to a strong infrared source. Hydroxyl (OH) radicals can be produced by photodissociation or collisional dissociation. H2O and OH can both be pumped to produce maser emission. OH masers in particular can give rise to a powerful maser action at 1612 MHz and this is regarded as a defining feature of the OH/IR stars. Many other AGB stars, such as Mira variables, show weaker OH masers at other wavelengths, such as 1667MHz or 22MHz.

Examples

OH/IR stars

OH/IR supergiants

Notes

References

Illustrations

OH/IR star: Very Large Telescope image of the surroundings of the red hypergiant VY Canis Majoris
Very Large Telescope image of the surroundings of the red hypergiant VY Canis Majoris

Worked examples

Example 1 — a first encounter with OH/IR star

Start with the simplest possible case. Write down what OH/IR star 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 OH/IR star 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 OH/IR star 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 OH/IR star

In research
OH/IR star 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 OH/IR star 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
OH/IR star is common in secondary-school and first-year university syllabi. It links to neighbouring topics Asymptotic-giant-branch stars, M-type giants, M-type hypergiants, so understanding it makes those chapters shorter.
In everyday life
Look for OH/IR star 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 OH/IR star in 20 minutes

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

Frequently asked questions

What is OH/IR star in simple terms?

An OH/IR star is an asymptotic giant branch (AGB), a red supergiant (RSG), or a red hypergiant (RHG) star that shows strong OH maser emission and is unusually bright at near-infrared wavelengths. In the very late stages of AGB evolution, a star develops a super-wind with extreme mass loss.

Why does OH/IR star 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 OH/IR star?

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 OH/IR star.

Tags

  • Asymptotic-giant-branch stars
  • M-type giants
  • M-type hypergiants
  • M-type supergiants
  • Star stubs
  • Star types
  • Stellar evolution

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