ArticleslgStudy

astronomy

Y Centauri

Y Centauri 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 Y Centauri rather than just read about it. In short: Y Centauri or Y Cen (HD 127233, HIP 70969) is a semiregular variable star in the constellation of Centaurus. The variability in the star was discovered by Williamina Fleming in 1895 and published in the Third Catalogue of Variable Stars.

Y Centauri — main illustration
Y Centauri — illustration

Key takeaways

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

Reference excerpt

Y Centauri or Y Cen (HD 127233, HIP 70969) is a semiregular variable star in the constellation of Centaurus. The variability in the star was discovered by Williamina Fleming in 1895 and published in the Third Catalogue of Variable Stars. The photographic magnitude range was given as 7.7 - 8.8, but the variability was described as "somewhat doubtful". It was later given the designation HV 52 in the Harvard Catalogue of Variable Stars. The General Catalogue of Variable Stars lists it as a semiregular variable star with a period of 180 days and a visual magnitude range of 8.0 - 9.1. A study of Hipparcos satellite photometry found a small amplitude range of 0.2 magnitudes at a visual magnitude of 8.53. The distance of the star is poorly known. The revised Hipparcos annual parallax of 3.50 mas gives a distance of 900 light years. A study taking into account the variability of the star found a parallax of 5.57 mas, corresponding to a distance of 585 light years. Both estimates have a margin of error over 20%. The Gaia Data Release 2 parallax lies between these two values and appears more accurate with a margin of error around 5%, but with a large value for astrometric noise. Gaia EDR3 does not list a parallax for this star. Y Centauri is an asymptotic giant branch star 330 times as luminous as the sun. Its spectral type varies between M4 and M7 as it pulsates. The star has been observed to produce 22 GHz water maser emission, although later searches did not find any maser emission.

References

Notes

Illustrations

Y Centauri illustration

Worked examples

Example 1 — a first encounter with Y Centauri

Start with the simplest possible case. Write down what Y Centauri 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 Y Centauri 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 Y Centauri 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 Y Centauri

In research
Y Centauri 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 Y Centauri 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
Y Centauri is common in secondary-school and first-year university syllabi. It links to neighbouring topics Astronomical objects discovered in 1895, Asymptotic-giant-branch stars, Centaurus, so understanding it makes those chapters shorter.
In everyday life
Look for Y Centauri 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.
Ask Teacher Smith questions about this articleOpens your AI tutor with a question about “Y Centauri” →

Affiliate

Preply — study more efficiently by working with a personal tutor. 50% off.

How to study Y Centauri in 20 minutes

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

Frequently asked questions

What is Y Centauri in simple terms?

Y Centauri or Y Cen (HD 127233, HIP 70969) is a semiregular variable star in the constellation of Centaurus. The variability in the star was discovered by Williamina Fleming in 1895 and published in the Third Catalogue of Variable Stars.

Why does Y Centauri 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 Y Centauri?

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 Y Centauri.

Tags

  • Astronomical objects discovered in 1895
  • Asymptotic-giant-branch stars
  • Centaurus
  • Discoveries by Williamina Fleming
  • Durchmusterung objects
  • Emission-line stars
  • Henry Draper Catalogue objects
  • Hipparcos objects
  • M-type giants
  • Objects with variable star designations
  • Semiregular variable stars

Keep exploring