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astronomy

NGC 5185

NGC 5185 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 5185 rather than just read about it. In short: NGC 5185 is a spiral galaxy in the constellation of Virgo. Its velocity with respect to the cosmic microwave background is 7,683±20 km/s, which corresponds to a Hubble distance of 369.6 ± 25.9 Mly (113.32 ± 7.94 Mpc).

NGC 5185 — main illustration
NGC 5185 — illustration

Key takeaways

  • NGC 5185 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 5185 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of NGC 5185 from memory before moving on to harder problems.

Reference excerpt

NGC 5185 is a spiral galaxy in the constellation of Virgo. Its velocity with respect to the cosmic microwave background is 7,683±20 km/s, which corresponds to a Hubble distance of 369.6 ± 25.9 Mly (113.32 ± 7.94 Mpc). Additionally, 16 non-redshift measurements give a similar mean distance of 374.23 ± 10.11 Mly (114.738 ± 3.101 Mpc). It was discovered by German-British astronomer William Herschel on 19 March 1787. NGC 5185 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.

LDC 985 Group NGC 5185 is a member of a group of galaxies known as LDC 985. The other five galaxies in the group are NGC 5181, NGC 5207, NGC 5221, NGC 5222, NGC 5230.

Supernovae Three supernovae have been observed in NGC 5185:

SN 2006br (Type Ia, mag. 17.8) was discovered by Tim Puckett and G. Sostero on 25 April 2006. SN 2006dz (type unknown, mag. 20.0) was discovered by the Carnegie Supernova Project on 31 May 2006. SN 2021gvm (Type II, mag. 19.5747) was discovered by the Zwicky Transient Facility on 21 March 2021.

See also List of NGC objects (5001–6000)

References

External links Media related to NGC 5185 at Wikimedia Commons NGC 5185 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images

Illustrations

NGC 5185 illustration

Worked examples

Example 1 — a first encounter with NGC 5185

Start with the simplest possible case. Write down what NGC 5185 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 5185 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 5185 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 5185

In research
NGC 5185 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 5185 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 5185 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Astronomical objects discovered in 1787, Discoveries by William Herschel, IRAS catalogue objects, so understanding it makes those chapters shorter.
In everyday life
Look for NGC 5185 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 5185 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what NGC 5185 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 5185 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is NGC 5185 in simple terms?

NGC 5185 is a spiral galaxy in the constellation of Virgo. Its velocity with respect to the cosmic microwave background is 7,683±20 km/s, which corresponds to a Hubble distance of 369.6 ± 25.9 Mly (113.32 ± 7.94 Mpc).

Why does NGC 5185 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 5185?

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 5185.

Tags

  • Astronomical objects discovered in 1787
  • Discoveries by William Herschel
  • IRAS catalogue objects
  • MCG objects
  • NGC objects
  • Principal Galaxies Catalogue objects
  • Seyfert galaxies
  • Spiral galaxies
  • UGC objects
  • Virgo (constellation)

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