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astronomy

Messier 86

Messier 86 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 Messier 86 rather than just read about it. In short: Messier 86 (also known as M86 or NGC 4406) is a bright elliptical or lenticular galaxy in the constellation of Virgo. It was discovered by Charles Messier in 1781.

Messier 86 — main illustration
Messier 86 — illustration

Key takeaways

  • Messier 86 belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect Messier 86 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of Messier 86 from memory before moving on to harder problems.

Reference excerpt

Messier 86 (also known as M86 or NGC 4406) is a bright elliptical or lenticular galaxy in the constellation of Virgo. It was discovered by Charles Messier in 1781. M86 lies in the heart of the Virgo Cluster of galaxies and forms a most conspicuous group with another large galaxy known as Messier 84. It displays the highest blue shift of all Messier objects, as it is, net of its other vectors of travel, approaching the Milky Way at 244 km/s. This is due to both galaxies falling roughly towards the center of the Virgo cluster from opposing ends. Messier 86 has a rich array of globular clusters, with a total number of around 3,800. Its halo also has a number of stellar streams interpreted as remnants of dwarf galaxies that have been disrupted and absorbed by this galaxy. Messier 86 is linked by several filaments of ionized gas to the severely disrupted spiral galaxy NGC 4438, indicating that M86 may have stripped some gas and interstellar dust from the spiral. It is also suffering ram-pressure stripping as it moves at high speed through Virgo's intracluster medium, losing its interstellar medium and leaving behind a very long trail of X ray-emitting hot gas that has been detected with the help of the Chandra space telescope. The metal composition of magnesium, silicon and sulfur in the M86 galaxy is more similar to the rest of the universe than its own stellar population. This suggests that even ram pressure stripping is insufficient to strip the inner parts of the galaxy.

See also List of Messier objects

References

External links

SEDS Lenticular Galaxy M86

Messier 86 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images

Illustrations

Messier 86 illustration

Worked examples

Example 1 — a first encounter with Messier 86

Start with the simplest possible case. Write down what Messier 86 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 Messier 86 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 Messier 86 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 Messier 86

In research
Messier 86 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 Messier 86 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
Messier 86 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Astronomical objects discovered in 1781, Discoveries by Charles Messier, Lenticular galaxies, so understanding it makes those chapters shorter.
In everyday life
Look for Messier 86 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 Messier 86 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what Messier 86 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 Messier 86 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Messier 86 in simple terms?

Messier 86 (also known as M86 or NGC 4406) is a bright elliptical or lenticular galaxy in the constellation of Virgo. It was discovered by Charles Messier in 1781.

Why does Messier 86 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 Messier 86?

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 Messier 86.

Tags

  • Astronomical objects discovered in 1781
  • Discoveries by Charles Messier
  • Lenticular galaxies
  • Messier objects
  • NGC objects
  • Principal Galaxies Catalogue objects
  • UGC objects
  • Virgo (constellation)
  • Virgo Cluster

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