astronomy

NGC 3362

NGC 3362 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 3362 rather than just read about it. In short: NGC 3362 is an intermediate spiral galaxy in the constellation of Leo. Its velocity with respect to the cosmic microwave background is 8676 ± 25 km/s, which corresponds to a Hubble distance of 127.97 ± 8.97 Mpc (~417 million light-years).

Key takeaways

NGC 3362 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 3362 to a quantity you can measure, compute or draw — that is where exam questions come from.
Reproduce the core statement of NGC 3362 from memory before moving on to harder problems.

Reference excerpt

NGC 3362 is an intermediate spiral galaxy in the constellation of Leo. Its velocity with respect to the cosmic microwave background is 8676 ± 25 km/s, which corresponds to a Hubble distance of 127.97 ± 8.97 Mpc (~417 million light-years). However, three non redshift measurements give a closer distance of 95.8 ± 3.984 Mpc (~312 million light-years). The galaxy was discovered by German astronomer Albert Marth on 22 March 1865. The SIMBAD database lists NGC 3362 as a Seyfert II Galaxy, i.e. it has a quasar-like nuclei with very high surface brightnesses whose spectra reveal strong, high-ionisation emission lines, but unlike quasars, the host galaxy is clearly detectable. The galaxies NGC 3362 and UGC 5892 are in the same region of the celestial sphere and about the same distance from the Milky Way. According to Abraham Mahtessian, they form a pair of galaxies.

Supernovae Three supernovae have been observed in NGC 3362:

SN 2001Y (Type II-P, mag. 18.1) was discovered by LOTOSS (Lick Observatory and Tenagra Observatory Supernova Searches) on 3 March 2001. SN 2010ct (Type II, mag. 19.2) was discovered by the Lick Observatory Supernova Search (LOSS) on 15 May 2010. SN 2019cda (Type Ic, mag. 18.1) was discovered by the Italian Supernovae Search Project (ISSP) on 24 March 2019.

Supermassive Black Hole According to the authors of a paper published in 2002, the mass of the central black hole of NGC 3362 is 5.89 x 10^6 M☉.

See also List of NGC objects (3001–4000)

References

External links Media related to NGC 3362 at Wikimedia Commons NGC 3362 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images

Illustrations

Worked examples

Example 1 — a first encounter with NGC 3362

Start with the simplest possible case. Write down what NGC 3362 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 3362 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 3362 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 3362

In research: NGC 3362 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 3362 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 3362 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Astronomical objects discovered in 1865, Discoveries by Albert Marth, Intermediate spiral galaxies, so understanding it makes those chapters shorter.
In everyday life: Look for NGC 3362 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 3362 in 20 minutes

Read the reference excerpt below once, without taking notes.
Close the page and write down what NGC 3362 means in your own words.
Compare your version with the excerpt and mark what you missed.
Work through the three examples above with pen and paper.
Explain NGC 3362 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is NGC 3362 in simple terms?

Why does NGC 3362 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 3362?

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 3362.