ArticleslgStudy

astronomy

V394 Aurigae

V394 Aurigae 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 V394 Aurigae rather than just read about it. In short: V394 Aurigae is a semi-regular variable star in the constellation Auriga. Its brightness varies between magnitudes 6.01 and 6.11, so it is faintly visible to the naked eye under ideal observing conditions.

V394 Aurigae — main illustration
V394 Aurigae — illustration

Key takeaways

  • V394 Aurigae belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect V394 Aurigae to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of V394 Aurigae from memory before moving on to harder problems.

Reference excerpt

V394 Aurigae is a semi-regular variable star in the constellation Auriga. Its brightness varies between magnitudes 6.01 and 6.11, so it is faintly visible to the naked eye under ideal observing conditions. Located around 880 light-years distant, V394 Aurigae shines with a luminosity approximately 985 times that of the Sun and has a surface temperature of 3,639 K. In 1991, Leroy F. Snyder discovered that the star, then called HR 2146, is a variable star. It was given its variable star designation, V394 Aurigae, in 1993. Koen and Eyer found that the star's brightness, as seen by Hipparcos, varies with a period of 3.9 days. It is a double star: the secondary, designated V394 Aurigae B, is an eleventh-magnitude F7V star with a separation of 10 arcseconds.

References

Illustrations

V394 Aurigae illustration
V394 Aurigae: A light curve for V394 Aurigae, plotted from Hipparcos data[8]
A light curve for V394 Aurigae, plotted from Hipparcos data[8]

Worked examples

Example 1 — a first encounter with V394 Aurigae

Start with the simplest possible case. Write down what V394 Aurigae 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 V394 Aurigae 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 V394 Aurigae 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 V394 Aurigae

In research
V394 Aurigae 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 V394 Aurigae 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
V394 Aurigae is common in secondary-school and first-year university syllabi. It links to neighbouring topics Asymptotic-giant-branch stars, Auriga, Bright Star Catalogue objects, so understanding it makes those chapters shorter.
In everyday life
Look for V394 Aurigae 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 “V394 Aurigae” →

Affiliate

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

How to study V394 Aurigae in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what V394 Aurigae 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 V394 Aurigae out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is V394 Aurigae in simple terms?

V394 Aurigae is a semi-regular variable star in the constellation Auriga. Its brightness varies between magnitudes 6.01 and 6.11, so it is faintly visible to the naked eye under ideal observing conditions.

Why does V394 Aurigae 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 V394 Aurigae?

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 V394 Aurigae.

Tags

  • Asymptotic-giant-branch stars
  • Auriga
  • Bright Star Catalogue objects
  • Double stars
  • Durchmusterung objects
  • F-type main-sequence stars
  • Henry Draper Catalogue objects
  • Hipparcos objects
  • M-type bright giants
  • Objects with variable star designations
  • Semiregular variable stars

Keep exploring