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UGC 11397

UGC 11397 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 UGC 11397 rather than just read about it. In short: UGC 11397 is a barred spiral galaxy in the constellation of Lyra. Its velocity with respect to the cosmic microwave background is 4,361±12 km/s, which corresponds to a Hubble distance of 209.8 ± 14.7 Mly (64.31 ± 4.51 Mpc).

UGC 11397 — main illustration
UGC 11397 — illustration

Key takeaways

  • UGC 11397 belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect UGC 11397 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of UGC 11397 from memory before moving on to harder problems.

Reference excerpt

UGC 11397 is a barred spiral galaxy in the constellation of Lyra. Its velocity with respect to the cosmic microwave background is 4,361±12 km/s, which corresponds to a Hubble distance of 209.8 ± 14.7 Mly (64.31 ± 4.51 Mpc). However, three non-redshift measurements give a farther distance of 257.66 ± 3.08 Mly (79.000 ± 0.945 Mpc). The first known reference to this galaxy comes from volume III of the Catalogue of Galaxies and of Clusters of Galaxies compiled by Fritz Zwicky in 1966, where it was listed as CGCG 202-003. UGC 11397 is a Seyfert II Galaxy, i.e. it has a quasar-like nucleus with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable. The center of UGC 11397 harbors a supermassive black hole, with a mass of 174 million M☉.

References

External links Media related to UGC 11397 at Wikimedia Commons UGC 11397 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images

Illustrations

UGC 11397 illustration

Worked examples

Example 1 — a first encounter with UGC 11397

Start with the simplest possible case. Write down what UGC 11397 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 UGC 11397 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 UGC 11397 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 UGC 11397

In research
UGC 11397 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 UGC 11397 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
UGC 11397 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Astronomical objects discovered in 1966, Barred spiral galaxies, IRAS catalogue objects, so understanding it makes those chapters shorter.
In everyday life
Look for UGC 11397 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 UGC 11397 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what UGC 11397 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 UGC 11397 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is UGC 11397 in simple terms?

UGC 11397 is a barred spiral galaxy in the constellation of Lyra. Its velocity with respect to the cosmic microwave background is 4,361±12 km/s, which corresponds to a Hubble distance of 209.8 ± 14.7 Mly (64.31 ± 4.51 Mpc).

Why does UGC 11397 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 UGC 11397?

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 UGC 11397.

Tags

  • Astronomical objects discovered in 1966
  • Barred spiral galaxies
  • IRAS catalogue objects
  • Lyra
  • Principal Galaxies Catalogue objects
  • Seyfert galaxies
  • UGC objects

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