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astronomy

NGC 1527

NGC 1527 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 1527 rather than just read about it. In short: NGC 1527 is a lenticular galaxy in the constellation of Horologium. Its velocity with respect to the cosmic microwave background is 1,178±17 km/s, which corresponds to a Hubble distance of 56.7 ± 4.1 Mly (17.37 ± 1.27 Mpc).

NGC 1527 — main illustration
NGC 1527 — illustration

Key takeaways

  • NGC 1527 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 1527 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of NGC 1527 from memory before moving on to harder problems.

Reference excerpt

NGC 1527 is a lenticular galaxy in the constellation of Horologium. Its velocity with respect to the cosmic microwave background is 1,178±17 km/s, which corresponds to a Hubble distance of 56.7 ± 4.1 Mly (17.37 ± 1.27 Mpc). Additionally, 10 non-redshift measurements give a mean distance of 55.87 ± 3.62 Mly (17.130 ± 1.111 Mpc). It was discovered by Scottish astronomer James Dunlop on 28 September 1826. NGC 1527 has a possible 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.

Galaxy group NGC 1527 is a member of a galaxy group known as HDC 257. The group contains at least 14 galaxies, including NGC 1433, NGC 1483, NGC 1487, NGC 1493, NGC 1494, NGC 1495, NGC 1510, NGC 1512, IC 1959, IC 2000 (galaxy), ESO 201-14, and two others.

Supernova One supernova has been observed in NGC 1527:

SN 2008ge (Type Iax, mag. 12.8) was discovered by The CHilean Automatic Supernova sEarch (CHASE) on 8 October 2008. It reached magnitude 12.2, making it the brightest supernova of 2008. It was initially classified as Type Ia, but later analysis concluded that it was Type Iax.

See also List of NGC objects (1001–2000)

References

External links Media related to NGC 1527 at Wikimedia Commons NGC 1527 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images

Illustrations

NGC 1527 illustration

Worked examples

Example 1 — a first encounter with NGC 1527

Start with the simplest possible case. Write down what NGC 1527 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 1527 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 1527 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 1527

In research
NGC 1527 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 1527 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 1527 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Astronomical objects discovered in 1826, Discoveries by James Dunlop, ESO objects, so understanding it makes those chapters shorter.
In everyday life
Look for NGC 1527 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 1527 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what NGC 1527 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 1527 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is NGC 1527 in simple terms?

NGC 1527 is a lenticular galaxy in the constellation of Horologium. Its velocity with respect to the cosmic microwave background is 1,178±17 km/s, which corresponds to a Hubble distance of 56.7 ± 4.1 Mly (17.37 ± 1.27 Mpc).

Why does NGC 1527 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 1527?

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 1527.

Tags

  • Astronomical objects discovered in 1826
  • Discoveries by James Dunlop
  • ESO objects
  • Horologium (constellation)
  • Lenticular galaxies
  • NGC objects
  • Principal Galaxies Catalogue objects

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