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astronomy

NGC 3621

NGC 3621 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 3621 rather than just read about it. In short: NGC 3621 is a disk spiral galaxy about 22 Mly (6.7 Mpc) away in the equatorial constellation of Hydra. It was discovered by German-British astronomer William Herschel on 17 February 1790.

NGC 3621 — main illustration
NGC 3621 — illustration

Key takeaways

  • NGC 3621 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 3621 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of NGC 3621 from memory before moving on to harder problems.

Reference excerpt

NGC 3621 is a disk spiral galaxy about 22 Mly (6.7 Mpc) away in the equatorial constellation of Hydra. It was discovered by German-British astronomer William Herschel on 17 February 1790. NGC 3621 is comparatively bright and can be well seen in moderate-sized telescopes. The galaxy is around 216,900 ly (66,500 pc) across and is inclined at an angle of 66° from being viewed face on. It shines with a luminosity equal to 13 billion times that of the Sun. The morphological classification is SA(s)d, which indicates this is an ordinary spiral with loosely wound arms. There is no evidence for a bulge. Although it appears to be isolated, NGC 3621 belongs to the Leo spur. This galaxy has an active nucleus that matches a Seyfert 2 optical spectrum, suggesting that a low mass supermassive black hole is present at the core. Based upon the motion of stars in the nucleus, this object may have a mass of up to three million times the mass of the Sun.

Supernova

One supernova has been observed in NGC 3621: SN 2024ggi (Type II, mag. 18.915) was discovered by ATLAS on 11 April 2024. By 16 April it had brightened to magnitude 12, and got as bright as magnitude 11.9, making it the brightest supernova of 2024. It was the closest supernova to Earth since SN 2023ixf, which had been discovered on 19 May 2023. A search of archival Hubble Space Telescope and Spitzer Space Telescope images showed the suspected progenitor star, identified as a red supergiant. The mass of the progenitor has been estimated at 12-15 M☉.

Gallery

See also List of NGC objects (3001–4000)

References

External links

A Picture-perfect Pure-disc Galaxy — ESO Photo release.

Illustrations

NGC 3621 illustration
NGC 3621: NGC 3621, with SN 2024ggi marked
NGC 3621, with SN 2024ggi marked
NGC 3621 illustration
NGC 3621 illustration
NGC 3621 illustration

Worked examples

Example 1 — a first encounter with NGC 3621

Start with the simplest possible case. Write down what NGC 3621 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 3621 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 3621 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 3621

In research
NGC 3621 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 3621 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 3621 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Astronomical objects discovered in 1790, Discoveries by William Herschel, ESO objects, so understanding it makes those chapters shorter.
In everyday life
Look for NGC 3621 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 3621 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what NGC 3621 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 3621 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is NGC 3621 in simple terms?

NGC 3621 is a disk spiral galaxy about 22 Mly (6.7 Mpc) away in the equatorial constellation of Hydra. It was discovered by German-British astronomer William Herschel on 17 February 1790.

Why does NGC 3621 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 3621?

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 3621.

Tags

  • Astronomical objects discovered in 1790
  • Discoveries by William Herschel
  • ESO objects
  • Field galaxies
  • Hydra (constellation)
  • IRAS catalogue objects
  • MCG objects
  • NGC objects
  • Principal Galaxies Catalogue objects
  • UGCA objects
  • Unbarred spiral galaxies

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