ArticleslgStudy

astronomy

NGC 5247

NGC 5247 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 NGC 5247 rather than just read about it. In short: NGC 5247 is a face-on unbarred spiral galaxy located some 60 million light years away in the constellation Virgo. It is a member of the Virgo II Groups, a series of galaxies and galaxy clusters strung out from the southern edge of the Virgo Supercluster.

NGC 5247 — main illustration
NGC 5247 — illustration

Key takeaways

  • NGC 5247 belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect NGC 5247 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of NGC 5247 from memory before moving on to harder problems.

Reference excerpt

NGC 5247 is a face-on unbarred spiral galaxy located some 60 million light years away in the constellation Virgo. It is a member of the Virgo II Groups, a series of galaxies and galaxy clusters strung out from the southern edge of the Virgo Supercluster. This is a grand design spiral galaxy that displays no indications of distortion caused by interaction with other galaxies. It has two spiral arms that bifurcate after wrapping halfway around the nucleus. The disk is estimated to be 4.9 ± 2.0 kly (1.5 ± 0.6 kpc) in thickness and it is inclined by roughly 28° to the line of sight.

Supernovae Two supernovae have been observed in NGC 5247:

PSN J13375721-1754272 (type II-P, mag. 15.6) was discovered by the Catalina Real-time Transient Survey on 24 July 2012. SN 2016C (type IIP, mag. 15.7) was discovered by Masakatsu Aoki on 3 January 2016.

References

External links Media related to NGC 5247 at Wikimedia Commons

NGC 5247 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images

Illustrations

NGC 5247 illustration
NGC 5247: NGC 5247 in ultraviolet by GALEX
NGC 5247 in ultraviolet by GALEX

Worked examples

Example 1 — a first encounter with NGC 5247

Start with the simplest possible case. Write down what NGC 5247 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 NGC 5247 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 NGC 5247 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 NGC 5247

In research
NGC 5247 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 NGC 5247 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
NGC 5247 is common in secondary-school and first-year university syllabi. It links to neighbouring topics NGC objects, Principal Galaxies Catalogue objects, UGCA objects, so understanding it makes those chapters shorter.
In everyday life
Look for NGC 5247 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.

Affiliate

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

How to study NGC 5247 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what NGC 5247 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 NGC 5247 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is NGC 5247 in simple terms?

NGC 5247 is a face-on unbarred spiral galaxy located some 60 million light years away in the constellation Virgo. It is a member of the Virgo II Groups, a series of galaxies and galaxy clusters strung out from the southern edge of the Virgo Supercluster.

Why does NGC 5247 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 NGC 5247?

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 NGC 5247.

Tags

  • NGC objects
  • Principal Galaxies Catalogue objects
  • UGCA objects
  • Unbarred spiral galaxies
  • Unbarred spiral galaxy stubs
  • Virgo (constellation)

Keep exploring