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astronomy

NGC 5876

NGC 5876 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 5876 rather than just read about it. In short: NGC 5876 is a barred spiral galaxy in the constellation of Boötes. Its velocity with respect to the cosmic microwave background is 3325 ± 5 km/s, which corresponds to a Hubble distance of 49.05 ± 3.43 Mpc (~160 million light-years).

NGC 5876 — main illustration
NGC 5876 — illustration

Key takeaways

  • NGC 5876 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 5876 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of NGC 5876 from memory before moving on to harder problems.

Reference excerpt

NGC 5876 is a barred spiral galaxy in the constellation of Boötes. Its velocity with respect to the cosmic microwave background is 3325 ± 5 km/s, which corresponds to a Hubble distance of 49.05 ± 3.43 Mpc (~160 million light-years). However, three non redshift measurements give a much greater distance of 65.6 ± 0.346 Mpc (~214 million light-years). The galaxy was discovered by American astronomer Lewis Swift on 11 June 1885. Swift observed the galaxy again on August 27, 1888, and not realizing that he had already observed it, entered the galaxy into the Index Catalogue as IC 1111. According to the SIMBAD database, NGC 5876 is a LINER galaxy, i.e. a galaxy whose nucleus has an emission spectrum characterized by broad lines of weakly ionized atoms.

NGC 5908 Group NGC 5876 is part of the NGC 5908 group (also known as LGG 395), which includes at least six other members: NGC 5820, NGC 5821, NGC 5874, NGC 5905, NGC 5908, and UGC 9759.

Supernova One supernova has been observed in NGC 5876: SN 2024igg (Type Ia-SC, mag. 17.7639) was discovered by the Automatic Learning for the Rapid Classification of Events (ALeRCE) on 7 May 2024.

See also List of NGC objects (5001–6000)

References

External links Media related to NGC 5876 at Wikimedia Commons NGC 5876 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images

Illustrations

NGC 5876 illustration

Worked examples

Example 1 — a first encounter with NGC 5876

Start with the simplest possible case. Write down what NGC 5876 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 5876 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 5876 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 5876

In research
NGC 5876 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 5876 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 5876 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Astronomical objects discovered in 1885, Barred spiral galaxies, Boötes, so understanding it makes those chapters shorter.
In everyday life
Look for NGC 5876 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 5876 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what NGC 5876 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 5876 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is NGC 5876 in simple terms?

NGC 5876 is a barred spiral galaxy in the constellation of Boötes. Its velocity with respect to the cosmic microwave background is 3325 ± 5 km/s, which corresponds to a Hubble distance of 49.05 ± 3.43 Mpc (~160 million light-years).

Why does NGC 5876 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 5876?

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 5876.

Tags

  • Astronomical objects discovered in 1885
  • Barred spiral galaxies
  • Boötes
  • Discoveries by Lewis Swift
  • IC objects
  • IRAS catalogue objects
  • LINER galaxies
  • MCG objects
  • NGC objects
  • Principal Galaxies Catalogue objects
  • UGC objects

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