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astronomy

NGC 1217

NGC 1217 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 1217 rather than just read about it. In short: NGC 1217 is a spiral galaxy in the constellation of Fornax. Its velocity with respect to the cosmic microwave background is 6,282±15 km/s, which corresponds to a Hubble distance of 302.2 ± 21.2 Mly (92.66 ± 6.49 Mpc).

NGC 1217 — main illustration
NGC 1217 — illustration

Key takeaways

  • NGC 1217 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 1217 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of NGC 1217 from memory before moving on to harder problems.

Reference excerpt

NGC 1217 is a spiral galaxy in the constellation of Fornax. Its velocity with respect to the cosmic microwave background is 6,282±15 km/s, which corresponds to a Hubble distance of 302.2 ± 21.2 Mly (92.66 ± 6.49 Mpc). Additionally, one non-redshift measurement provides a much closer distance estimate of 199.93 Mly (61.300 Mpc). It was discovered by British astronomer John Herschel on 23 October 1835. NGC 1217 has an active galactic nucleus, i.e. it has a compact region at the center of a galaxy that emits a significant amount of energy across the electromagnetic spectrum, with characteristics indicating that this luminosity is not produced by the stars. NGC 1217 is also 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. It is also a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms.

Supernova One supernova has been observed in NGC 1217:

SN 2025ygq (Type Ia, mag. 18.483) was discovered by ATLAS on 22 September 2025.

See also List of NGC objects (1001–2000)

References

External links Media related to NGC 1217 at Wikimedia Commons NGC 1217 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images

Illustrations

NGC 1217 illustration

Worked examples

Example 1 — a first encounter with NGC 1217

Start with the simplest possible case. Write down what NGC 1217 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 1217 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 1217 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 1217

In research
NGC 1217 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 1217 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 1217 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Astronomical objects discovered in 1835, Discoveries by John Herschel, ESO objects, so understanding it makes those chapters shorter.
In everyday life
Look for NGC 1217 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 NGC 1217 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what NGC 1217 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 1217 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is NGC 1217 in simple terms?

NGC 1217 is a spiral galaxy in the constellation of Fornax. Its velocity with respect to the cosmic microwave background is 6,282±15 km/s, which corresponds to a Hubble distance of 302.2 ± 21.2 Mly (92.66 ± 6.49 Mpc).

Why does NGC 1217 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 1217?

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 1217.

Tags

  • Astronomical objects discovered in 1835
  • Discoveries by John Herschel
  • ESO objects
  • Fornax
  • IRAS catalogue objects
  • LINER galaxies
  • MCG objects
  • NGC objects
  • Principal Galaxies Catalogue objects
  • Seyfert galaxies
  • Spiral galaxies

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