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astronomy

NGC 759

NGC 759 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 759 rather than just read about it. In short: NGC 759 is an elliptical galaxy located 230 million light-years away in the constellation Andromeda. NGC 759 was discovered by astronomer by Heinrich d'Arrest on September 17, 1865.

NGC 759 — main illustration
NGC 759 — illustration

Key takeaways

  • NGC 759 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 759 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of NGC 759 from memory before moving on to harder problems.

Reference excerpt

NGC 759 is an elliptical galaxy located 230 million light-years away in the constellation Andromeda. NGC 759 was discovered by astronomer by Heinrich d'Arrest on September 17, 1865. It is a member of Abell 262. Despite being classified as a radio galaxy, the radio emission in NGC 759 could be due to star formation rather than an active galactic nucleus.

Dust disk The central region of NGC 759 harbors a face-on dust disk with tightly wound spiral structure. The disk has a diameter of 11,000 ly (3.4 kpc). The dust disk also contains a smaller circumnuclear molecular gas ring that has star formation in H II regions. These features may be the result of a merger of gas-rich disk galaxies or by the accretion of gas-rich material. In either scenario, the gas would have lost momentum and fallen to the center of the galaxy to produce the disk and current star formation. However, Vlasyuk et al. suggests that the disk and the smaller circumnuclear molecular gas ring with star formation inside the main disk formed from a tidal encounter between NGC 759 and a large spiral galaxy which was accompanied by a substantial gas accretion.

Molecular gas NGC 759 contains 2.4 billion M☉ of molecular gas. Most of the gas is concentrated in a circumnuclear molecular gas ring with a diameter of 4,200 ly (1.3 kpc). The gas may be the result of the same merger event that produced the circumnuclear molecular gas ring and the main disk.

Supernova One supernova has been observed in NGC 759.

SN 2002fb (Type Ia, mag. 17.1) was discovered by LOTOSS (Lick Observatory and Tenagra Observatory Supernova Searches) on September 6, 2002.

See also List of NGC objects (1–1000)

References

External links

NGC 759 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images

Illustrations

NGC 759 illustration
NGC 759: The dust disk in NGC 759 as imaged by the Hubble Space Telescope
The dust disk in NGC 759 as imaged by the Hubble Space Telescope

Worked examples

Example 1 — a first encounter with NGC 759

Start with the simplest possible case. Write down what NGC 759 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 759 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 759 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 759

In research
NGC 759 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 759 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 759 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Abell 262, Andromeda (constellation), Astronomical objects discovered in 1865, so understanding it makes those chapters shorter.
In everyday life
Look for NGC 759 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 759 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what NGC 759 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 759 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is NGC 759 in simple terms?

NGC 759 is an elliptical galaxy located 230 million light-years away in the constellation Andromeda. NGC 759 was discovered by astronomer by Heinrich d'Arrest on September 17, 1865.

Why does NGC 759 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 759?

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 759.

Tags

  • Abell 262
  • Andromeda (constellation)
  • Astronomical objects discovered in 1865
  • Elliptical galaxies
  • NGC objects
  • Principal Galaxies Catalogue objects
  • Radio galaxies
  • UGC objects

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