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astronomy

NGC 3052

NGC 3052 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 3052 rather than just read about it. In short: NGC 3052 is an intermediate spiral galaxy in the constellation of Hydra. Its velocity concerning the cosmic microwave background is 4122 ± 24 km/s, which corresponds to a Hubble distance of 60.79 ± 4.27 Mpc (~198 million light-years).

NGC 3052 — main illustration
NGC 3052 — illustration

Key takeaways

  • NGC 3052 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 3052 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of NGC 3052 from memory before moving on to harder problems.

Reference excerpt

NGC 3052 is an intermediate spiral galaxy in the constellation of Hydra. Its velocity concerning the cosmic microwave background is 4122 ± 24 km/s, which corresponds to a Hubble distance of 60.79 ± 4.27 Mpc (~198 million light-years). However, 19 nonredshift measurements give a much closer distance of 42.563 ± 6.434 Mpc (139 million light-years). The galaxy was discovered by German-British astronomer William Herschel on 7 February 1785. The SIMBAD database lists NGC 3052 as a Seyfert I Galaxy, i.e. it has a quasar-like nuclei with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable. One supernova has been observed in NGC 3052: SN 2024chx (Type II, mag. 18.2315) was discovered by the Zwicky Transient Facility on 12 February 2024.

NGC 3091 Group The galaxy NGC 3052 is part of the NGC 3091 group (also known as LGG 186), which includes at least 5 other galaxies: NGC 3091, NGC 3124, PGC 28926, MCG -3-26-6, and ESO 566–19.

See also List of NGC objects (3001–4000)

References

External links Media related to NGC 3052 at Wikimedia Commons NGC 3052 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images

Illustrations

NGC 3052 illustration

Worked examples

Example 1 — a first encounter with NGC 3052

Start with the simplest possible case. Write down what NGC 3052 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 3052 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 3052 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 3052

In research
NGC 3052 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 3052 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 3052 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Astronomical objects discovered in 1785, Discoveries by William Herschel, ESO objects, so understanding it makes those chapters shorter.
In everyday life
Look for NGC 3052 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 3052 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what NGC 3052 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 3052 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is NGC 3052 in simple terms?

NGC 3052 is an intermediate spiral galaxy in the constellation of Hydra. Its velocity concerning the cosmic microwave background is 4122 ± 24 km/s, which corresponds to a Hubble distance of 60.79 ± 4.27 Mpc (~198 million light-years).

Why does NGC 3052 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 3052?

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 3052.

Tags

  • Astronomical objects discovered in 1785
  • Discoveries by William Herschel
  • ESO objects
  • Hydra (constellation)
  • IRAS catalogue objects
  • Intermediate spiral galaxies
  • MCG objects
  • NGC objects
  • Principal Galaxies Catalogue objects
  • Seyfert galaxies

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