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astronomy

R Leonis

R Leonis 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 R Leonis rather than just read about it. In short: R Leonis is a red giant Mira-type variable star located approximately 370 light years away in the constellation Leo. The apparent magnitude of R Leonis varies between 4.31 and 11.65 with a period of 312 days.

R Leonis — main illustration
R Leonis — illustration

Key takeaways

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

Reference excerpt

R Leonis is a red giant Mira-type variable star located approximately 370 light years away in the constellation Leo.

The apparent magnitude of R Leonis varies between 4.31 and 11.65 with a period of 312 days. At maximum it can be seen with the naked eye, while at minimum a telescope of at least 7 cm is needed. The star's effective temperature is estimated to be 2,930 – 3,080 kelvins and radius spans 320 solar radii (220,000,000 kilometres; 1.5 astronomical units), roughly Mars's orbital zone.

Possible planet

In 2009 Wiesemeyer et al. proposed that quasi-periodic fluctuations observed for the star R Leonis may be due to the presence of an evaporating substellar companion, probably an extrasolar planet. They have inferred a putative mass for the orbiting body of twice the mass of Jupiter, orbital period of 5.2 years and likely orbital separation of 2.7 astronomical units. If confirmed such a planetary object could likely be an evaporating planet, with a long comet-like trail as hinted by intense SiO maser emissions.

References

External links AAVSO Variable Star of the Month. April, 2001: R Leonis Archived 2003-11-06 at the Wayback Machine

Illustrations

R Leonis illustration
R Leonis: The light curve of R Leonis from AAVSO V band data[7]
The light curve of R Leonis from AAVSO V band data[7]
R Leonis: Artistic rendering of R Leonis's putative evaporating planetary companion
Artistic rendering of R Leonis's putative evaporating planetary companion

Worked examples

Example 1 — a first encounter with R Leonis

Start with the simplest possible case. Write down what R Leonis 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 R Leonis 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 R Leonis 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 R Leonis

In research
R Leonis 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 R Leonis 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
R Leonis is common in secondary-school and first-year university syllabi. It links to neighbouring topics Bright Star Catalogue objects, Durchmusterung objects, Emission-line stars, so understanding it makes those chapters shorter.
In everyday life
Look for R Leonis 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 R Leonis in 20 minutes

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

Frequently asked questions

What is R Leonis in simple terms?

R Leonis is a red giant Mira-type variable star located approximately 370 light years away in the constellation Leo. The apparent magnitude of R Leonis varies between 4.31 and 11.65 with a period of 312 days.

Why does R Leonis 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 R Leonis?

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 R Leonis.

Tags

  • Bright Star Catalogue objects
  • Durchmusterung objects
  • Emission-line stars
  • Henry Draper Catalogue objects
  • Hipparcos objects
  • Hypothetical planetary systems
  • Leo (constellation)
  • M-type giants
  • Mira variables
  • Objects with variable star designations

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