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UW Canis Majoris

UW 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 UW Canis Majoris rather than just read about it. In short: UW Canis Majoris is a star in the constellation Canis Major. It is classified as a Beta Lyrae eclipsing contact binary and given the variable star designation UW Canis Majoris.

UW Canis Majoris — main illustration
UW Canis Majoris — illustration

Key takeaways

  • UW 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 UW Canis Majoris to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of UW Canis Majoris from memory before moving on to harder problems.

Reference excerpt

UW Canis Majoris is a star in the constellation Canis Major. It is classified as a Beta Lyrae eclipsing contact binary and given the variable star designation UW Canis Majoris. Its brightness varies from magnitude +4.84 to +5.33 with a period of 4.39 days. Bode had initially labelled it as Tau2 Canis Majoris, but this designation had been dropped by Gould and subsequent authors. It is visible to the naked eye of a person under good observing conditions. Sergai Gaposchnhkin analyzed 376 photographic plates taken over a twelve year period, and announced in 1936 that 29 Canis Majoris is a variable star. It was given its variable star designation in 1936.

UW Canis Majoris A is a rare blue supergiant of spectral type O7.5-8 Iab. The precise characteristics of the system are still uncertain, in part because the spectral signature of the secondary is very hard to disentangle from the spectrum of the primary and the surrounding envelope of stellar wind. A detailed spectral study by Gies et al. found that the primary had a diameter 13 times that of the Sun, while its secondary companion is a slightly cooler, less evolved and less luminous supergiant of spectral type O9.7Ib that is 10 times the Sun's diameter. According to this study, the brighter star is the more luminous, its luminosity 200,000 times that of the Sun as opposed to the secondary's 63,000 times. However the secondary is the more massive star at 19 Solar masses (M☉) compared to the primary's 16 M☉. However, a more recent photometric analysis finds several configurations of mass and luminosity ratios that match the observed data. Parallax measurements showed it to be approximately 3,000 light years from Earth, but this is unexpectedly close for a star of its spectral type and brightness. More accurate Hipparcos parallax data gives an even closer result around 2000 light years, but Gaia Data Release 3 gives a parallax of 0.85±0.13 mas, corresponding to a distance of around 3,800 light years. It is thought to be a distant member of NGC 2362 which would place it about 5,000 light years and more closely match its expected luminosity. The contradiction between the different distance results is still a subject of research. UW Canis Majoris is part of the giant HII Region Sh2-310 and it along with Tau Canis Majoris which is the brightest member of NGC 2362, HD 58011, and VY Canis Majoris are thought to be are thought to be probable sources of ionization of gases in Sh2-310.

References

Illustrations

UW Canis Majoris illustration
UW Canis Majoris: NGC 2362 with UW CMa at the top (north) of the frame
NGC 2362 with UW CMa at the top (north) of the frame
UW Canis Majoris: A light curve for UW Canis Majoris from Hipparcos data, adapted from Antokhina et al. (2011)[7]
A light curve for UW Canis Majoris from Hipparcos data, adapted from Antokhina et al. (2011)[7]

Worked examples

Example 1 — a first encounter with UW Canis Majoris

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

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

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

Frequently asked questions

What is UW Canis Majoris in simple terms?

UW Canis Majoris is a star in the constellation Canis Major. It is classified as a Beta Lyrae eclipsing contact binary and given the variable star designation UW Canis Majoris.

Why does UW 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 UW 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 UW Canis Majoris.

Tags

  • Beta Lyrae variables
  • Bright Star Catalogue objects
  • Canis Major
  • Durchmusterung objects
  • Emission-line stars
  • Flamsteed objects
  • Henry Draper Catalogue objects
  • Hipparcos objects
  • O-type supergiants
  • Objects with variable star designations
  • Sh 2-310

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