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astronomy

NGC 6106

NGC 6106 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 6106 rather than just read about it. In short: NGC 6106 is a spiral galaxy in the constellation of Hercules. Its velocity with respect to the cosmic microwave background is 1,527±6 km/s, which corresponds to a Hubble distance of 73.5 ± 5.2 Mly (22.52 ± 1.58 Mpc).

NGC 6106 — main illustration
NGC 6106 — illustration

Key takeaways

  • NGC 6106 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 6106 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of NGC 6106 from memory before moving on to harder problems.

Reference excerpt

NGC 6106 is a spiral galaxy in the constellation of Hercules. Its velocity with respect to the cosmic microwave background is 1,527±6 km/s, which corresponds to a Hubble distance of 73.5 ± 5.2 Mly (22.52 ± 1.58 Mpc). This is in good agreement with 29 non-redshift measurements which give an average distance of 72.64 ± 2.49 Mly (22.272 ± 0.764 Mpc). It was discovered by German-British astronomer William Herschel on 13 April 1784. NGC 6106 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.

Luminous red nova and supernova

One luminous red nova and one supernova have been observed in NGC 6106:

AT 2020kog (type LRN, mag. 20.3) was discovered by Panoramic Survey Telescope and Rapid Response System (Pan-STARRS) Search for Kilonovae on 18 May 2020. SN 2024ahv (Type Ib, mag. 16.2) was discovered by Japanese astronomer Hidehiko Okoshi on 16 January 2024.

See also List of NGC objects (6001–7000)

References

External links Media related to NGC 6106 at Wikimedia Commons NGC 6106 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images

Illustrations

NGC 6106 illustration
NGC 6106: The luminous red nova AT 2020kog imaged by the James Webb Space Telescope's MIRI
The luminous red nova AT 2020kog imaged by the James Webb Space Telescope's MIRI

Worked examples

Example 1 — a first encounter with NGC 6106

Start with the simplest possible case. Write down what NGC 6106 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 6106 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 6106 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 6106

In research
NGC 6106 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 6106 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 6106 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Astronomical objects discovered in 1784, Discoveries by William Herschel, Hercules (constellation), so understanding it makes those chapters shorter.
In everyday life
Look for NGC 6106 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 6106 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what NGC 6106 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 6106 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is NGC 6106 in simple terms?

NGC 6106 is a spiral galaxy in the constellation of Hercules. Its velocity with respect to the cosmic microwave background is 1,527±6 km/s, which corresponds to a Hubble distance of 73.5 ± 5.2 Mly (22.52 ± 1.58 Mpc).

Why does NGC 6106 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 6106?

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 6106.

Tags

  • Astronomical objects discovered in 1784
  • Discoveries by William Herschel
  • Hercules (constellation)
  • IRAS catalogue objects
  • MCG objects
  • NGC objects
  • Principal Galaxies Catalogue objects
  • Spiral galaxies
  • UGC objects

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