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astronomy

Sigma Canis Majoris

Sigma Canis Majoris 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 Sigma Canis Majoris rather than just read about it. In short: Sigma Canis Majoris is a variable star in the southern constellation of Canis Major. It has the proper name Nganurganity [ˈŋanuɾˌɡ̊aniɟ̊] (historically written Unurgunite ); Sigma Canis Majoris is its Bayer designation.

Sigma Canis Majoris — main illustration
Sigma Canis Majoris — illustration

Key takeaways

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

Reference excerpt

Sigma Canis Majoris is a variable star in the southern constellation of Canis Major. It has the proper name Nganurganity [ˈŋanuɾˌɡ̊aniɟ̊] (historically written Unurgunite ); Sigma Canis Majoris is its Bayer designation. This star is located at a distance of approximately 1,290 light-years (400 parsecs) from the Sun. It has an apparent visual magnitude varying between 3.43 and 3.51, which is bright enough to be seen with the naked eye. The star is drifting further away with a line of sight velocity of +22 km/s.

Nomenclature σ Canis Majoris (Latinised to Sigma Canis Majoris, abbreviated Sigma CMa, σ CMa) is the system's Bayer designation. The star is identified with the nganurganity [ˈŋanuɾˌɡ̊aniɟ̊] "Jacky lizard" in the culture of the Boorong, a clan of the indigenous Maligundidj people of northwestern Victoria in Australia, who saw it as an ancestral figure who fights the Moon, flanked by his wives (the stars Delta and Epsilon Canis Majoris). The name was transcribed by settler William Stanbridge as "Unurgunite" in the 1850s. (Initial ng-, which does not occur in English, was typically ignored in transcription of that era.) In 2016, the International Astronomical Union organized a Working Group on Star Names (WGSN) to catalog and standardize proper names for stars. The WGSN approved the name Unurgunite for σ Canis Majoris on 5 September 2017 and it is now so included in the List of IAU-approved Star Names. The spelling was later corrected to "Nganurganity". (Other historical corruptions of star names, such as Betelgeuse, are accepted as correct forms.)

Properties Sigma Canis Majoris is a supergiant star with a stellar classification of K5 Ib. This is a type of star that is in the late stages of its evolution, having consumed the hydrogen at its core and ballooned out to 290 times the Sun's radius. At 1.38 astronomical units, this radius is 38% larger than the average distance of the Earth from the Sun. It is currently radiating more than 15,800 times the luminosity of the Sun from its outer envelope at an effective temperature of around 3,800 K. This temperature gives it the cool orange-red hue of a late K-type star.

Sigma Canis Majoris was noted as a likely variable star in a list of bright southern stars studied at the Cape Observatory. The variability was confirmed in 1963, and it was formally catalogued as a variable star. It is classified as an irregular variable star and its brightness varies from magnitude +3.43 to +3.51. The magnetic field of this star has a strength below 1 G. It is suspected of being a member of the Collinder 121 stellar association of co-moving stars, but this is disputed. Sigma Canis Majoris is listed as a potential type II supernova progenitor. Instruments are capable of measuring the pre-supernova neutrino flux that could act as an alert that the supernova explosion was starting.

References

Illustrations

Sigma Canis Majoris illustration
Sigma Canis Majoris: A light curve for Sigma Canis Majoris, plotted from Hipparcos data
A light curve for Sigma Canis Majoris, plotted from Hipparcos data

Worked examples

Example 1 — a first encounter with Sigma Canis Majoris

Start with the simplest possible case. Write down what Sigma Canis Majoris 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 Sigma Canis Majoris 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 Sigma Canis Majoris 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 Sigma Canis Majoris

In research
Sigma Canis Majoris 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 Sigma Canis Majoris 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
Sigma Canis Majoris is common in secondary-school and first-year university syllabi. It links to neighbouring topics Bayer objects, Bright Star Catalogue objects, Canis Major, so understanding it makes those chapters shorter.
In everyday life
Look for Sigma Canis Majoris 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 Sigma Canis Majoris in 20 minutes

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

Frequently asked questions

What is Sigma Canis Majoris in simple terms?

Sigma Canis Majoris is a variable star in the southern constellation of Canis Major. It has the proper name Nganurganity [ˈŋanuɾˌɡ̊aniɟ̊] (historically written Unurgunite ); Sigma Canis Majoris is its Bayer designation.

Why does Sigma Canis Majoris 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 Sigma Canis Majoris?

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 Sigma Canis Majoris.

Tags

  • Bayer objects
  • Bright Star Catalogue objects
  • Canis Major
  • Durchmusterung objects
  • Flamsteed objects
  • Henry Draper Catalogue objects
  • Hipparcos objects
  • K-type giants
  • Population I stars
  • Slow irregular variables
  • Stars with proper names

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