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NGC 1396

NGC 1396 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 1396 rather than just read about it. In short: NGC 1396 is a dwarf elliptical galaxy located 61 million light years away in the constellation of Fornax. The galaxy was discovered by astronomer Julius Schmidt on January 19, 1865, and is a member of the Fornax Cluster.

NGC 1396 — main illustration
NGC 1396 — illustration

Key takeaways

  • NGC 1396 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 1396 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of NGC 1396 from memory before moving on to harder problems.

Reference excerpt

NGC 1396 is a dwarf elliptical galaxy located 61 million light years away in the constellation of Fornax. The galaxy was discovered by astronomer Julius Schmidt on January 19, 1865, and is a member of the Fornax Cluster. Despite the fact that the galaxy PGC 13398 is most commonly identified as NGC 1396, there is uncertainty in its identification. NGC 1396 is a satellite galaxy of NGC 1399. 232 known globular clusters have been observed surrounding NGC 1396, along with a central nuclear star cluster with an estimated mass of 9.6 million M☉. NGC 1396 has a metallicity of [Fe/H]~ -0.4, with unusually overabundant values of [Ca/Fe] ~+ 0.1, and underabundant sodium, with [Na/Fe] values around -0.1, while [Mg/Fe] is overabundant throughout the galaxy, increasing at a greater distance from the center of the galaxy. These abundance ratios compared with galaxies in the Local Group, show that the chemical enrichment history of the interstellar medium of NGC 1396 is similar to the galactic disc of the Milky Way. This implies that NGC 1396 originated as a progenitor galaxy the size of the Large Magellanic Cloud that lost its gas as it fell though the Fornax Cluster.

See also List of NGC objects (1001–2000) Messier 32 Messier 110

External links NGC 1396 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images

References

Illustrations

NGC 1396 illustration

Worked examples

Example 1 — a first encounter with NGC 1396

Start with the simplest possible case. Write down what NGC 1396 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 1396 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 1396 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 1396

In research
NGC 1396 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 1396 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 1396 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Astronomical objects discovered in 1865, Dwarf elliptical galaxies, Fornax, so understanding it makes those chapters shorter.
In everyday life
Look for NGC 1396 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 1396 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what NGC 1396 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 1396 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is NGC 1396 in simple terms?

NGC 1396 is a dwarf elliptical galaxy located 61 million light years away in the constellation of Fornax. The galaxy was discovered by astronomer Julius Schmidt on January 19, 1865, and is a member of the Fornax Cluster.

Why does NGC 1396 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 1396?

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 1396.

Tags

  • Astronomical objects discovered in 1865
  • Dwarf elliptical galaxies
  • Fornax
  • Fornax Cluster
  • NGC objects
  • Principal Galaxies Catalogue objects

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