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WX Coronae Australis

WX Coronae Australis 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 WX Coronae Australis rather than just read about it. In short: WX Coronae Australis (WX CrA) is an R Coronae Borealis (R CrB) star in the constellation Corona Australis, one of the brightest examples of this extremely rare class of variable star. Despite the rarity, Corona Australis hosts another R CrB star, V Coronae Australis.

WX Coronae Australis — main illustration
WX Coronae Australis — illustration

Key takeaways

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

Reference excerpt

WX Coronae Australis (WX CrA) is an R Coronae Borealis (R CrB) star in the constellation Corona Australis, one of the brightest examples of this extremely rare class of variable star. Despite the rarity, Corona Australis hosts another R CrB star, V Coronae Australis. WX Coronae Australis is a luminous star with a large excess of carbon and very little hydrogen. It has the spectrum of a carbon star, of type R5 indicating that it shows strong carbon molecular bands but not as red overall as the majority of carbon stars. Its brightness is variable, with 78.9-day pulsations producing changes of about 0.1 magnitudes, as well as occasional deep fades by six or more magnitudes. This classifies it as an R Coronae Borealis variable. These stars are likely to have formed from the merger of two white dwarfs into a hydrogen-deficient carbon-rich hot supergiant that then cooled. The deep fades are caused by obscuration by carbon-rich dust condensing around the star. WX Coronae Australis was first reported to be variable in 1928 after it was detected on two different photographic plates at magnitudes 12.2 and 16.0. It was catalogued as HV (Harvard Variable) 4119. The type of variability was not known at the time, but in 1936 its spectrum was measured as R5 and it was tentatively classified as an R CrB star. By 1996 it had been observed to fade 13 times at an average interval of 2,000 days.

References

Illustrations

WX Coronae Australis illustration

Worked examples

Example 1 — a first encounter with WX Coronae Australis

Start with the simplest possible case. Write down what WX Coronae Australis 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 WX Coronae Australis 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 WX Coronae Australis 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 WX Coronae Australis

In research
WX Coronae Australis 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 WX Coronae Australis 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
WX Coronae Australis is common in secondary-school and first-year university syllabi. It links to neighbouring topics Carbon stars, Corona Australis, Durchmusterung objects, so understanding it makes those chapters shorter.
In everyday life
Look for WX Coronae Australis 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 WX Coronae Australis in 20 minutes

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

Frequently asked questions

What is WX Coronae Australis in simple terms?

WX Coronae Australis (WX CrA) is an R Coronae Borealis (R CrB) star in the constellation Corona Australis, one of the brightest examples of this extremely rare class of variable star. Despite the rarity, Corona Australis hosts another R CrB star, V Coronae Australis.

Why does WX Coronae Australis 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 WX Coronae Australis?

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 WX Coronae Australis.

Tags

  • Carbon stars
  • Corona Australis
  • Durchmusterung objects
  • Henry Draper Catalogue objects
  • Objects with variable star designations
  • R Coronae Borealis variables

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