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Messier 96

Messier 96 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 96 rather than just read about it. In short: Messier 96 (also known as M96 or NGC 3368) is an intermediate spiral galaxy about 31 million light-years away in the constellation Leo. Observational history and appearance M96 was discovered by French astronomer Pierre Méchain on March 20, 1781.

Messier 96 — main illustration
Messier 96 — illustration

Key takeaways

  • Messier 96 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 96 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of Messier 96 from memory before moving on to harder problems.

Reference excerpt

Messier 96 (also known as M96 or NGC 3368) is an intermediate spiral galaxy about 31 million light-years away in the constellation Leo.

Observational history and appearance M96 was discovered by French astronomer Pierre Méchain on March 20, 1781. After communicating his finding, French astronomer Charles Messier confirmed the finding four days later and added it to his catalogue of nebulous objects. Finding this object is burdensome with large binoculars. Ideal minimum resolution, in a good sky, is via a telescope of 25.4 cm (10.0 in) aperture, to reveal its three-by-five-arcminute halo with a brighter core region. This complex galaxy is inclined by an angle of about 53° to the line of sight from the Earth, which is oriented at a position angle of 172°.

Properties

Messier 96 is categorized as a double-barred spiral galaxy with a small inner bulge through the core along with an outer bulge. The nucleus displays a weak level of activity of the LINER2 type. Variations in ultraviolet emission from the core suggest the presence of a supermassive black hole. Estimates for the mass of this object range from 1.5×106 to 4.8×107 solar masses (M☉). Messier 96 is about the same mass and size as the Milky Way. It is a very asymmetric galaxy; its dust and gas are unevenly spread throughout its weak spiral arms, and its core is just offset from the midpoint of its extremes. Its arms are also asymmetrical, thought to have been influenced by the gravitational pull of other galaxies within its group. Messier 96 is being studied as part of a survey of 50 nearby galaxies known as the Legacy ExtraGalactic UV Survey (LEGUS), providing an unprecedented view of star formation within the local universe.

Supernova

One supernova has been observed in M96. SN 1998bu (Type Ia, mag. 13) was discovered by Mirko Villi on May 9, 1998. It reached maximum brightness on May 21 at about magnitude 11.6, making it the brightest supernova of 1998, then steadily faded. Observations of the ejecta a year later showed creation of 0.4 solar masses of iron. The spectrum of the supernova remnant confirmed radioactive 56Co, which decays into 56Fe.

M96 group

M96 is the brightest galaxy within the M96 Group, a group of galaxies in Leo, the other Messier objects of which are M95 and M105. To this are added at least nine other galaxies. This is the nearest group to the Local Group to combine bright spirals and a bright elliptical galaxy (Messier 105).

See also List of Messier objects

References

External links

Messier 96 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images NOAO: M96 Archived 2014-08-11 at the Wayback Machine SEDS: Spiral Galaxy M96 Gray, Meghan; Hardy, Liam. "M96 – Spiral Galaxy". Deep Sky Videos. Brady Haran.

Illustrations

Messier 96 illustration
Messier 96: ESO's Very Large Telescope image of Messier 96. It shows its core displaced from the centre, its gas and dust are distributed asymmetrically and its spiral arms are ill-defined.
ESO's Very Large Telescope image of Messier 96. It shows its core displaced from the centre, its gas and dust are distributed asymmetrically and its spiral arms are ill-defined.
Messier 96: M96 with SN 1998bu imaged by the Cerro Tololo Inter-American Observatory
M96 with SN 1998bu imaged by the Cerro Tololo Inter-American Observatory

Worked examples

Example 1 — a first encounter with Messier 96

Start with the simplest possible case. Write down what Messier 96 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 96 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 96 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 96

In research
Messier 96 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 96 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 96 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Astronomical objects discovered in 1781, Discoveries by Pierre Méchain, IRAS catalogue objects, so understanding it makes those chapters shorter.
In everyday life
Look for Messier 96 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 96 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what Messier 96 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 96 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Messier 96 in simple terms?

Messier 96 (also known as M96 or NGC 3368) is an intermediate spiral galaxy about 31 million light-years away in the constellation Leo. Observational history and appearance M96 was discovered by French astronomer Pierre Méchain on March 20, 1781.

Why does Messier 96 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 96?

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 96.

Tags

  • Astronomical objects discovered in 1781
  • Discoveries by Pierre Méchain
  • IRAS catalogue objects
  • Intermediate spiral galaxies
  • Leo (constellation)
  • M96 Group
  • MCG objects
  • Messier objects
  • NGC objects
  • Principal Galaxies Catalogue objects
  • UGC objects

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