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SDSS J092048.27+302818.3

SDSS J092048.27+302818.3 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 SDSS J092048.27+302818.3 rather than just read about it. In short: SDSS J092048.27+302818.3 also known as OGC 330 and SHELS J140.2012763+30.4717820 is a elliptical galaxy located in the constellation of Cancer. The redshift of the galaxy is (z) 0.288.

SDSS J092048.27+302818.3 — main illustration
SDSS J092048.27+302818.3 — illustration

Key takeaways

  • SDSS J092048.27+302818.3 belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect SDSS J092048.27+302818.3 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of SDSS J092048.27+302818.3 from memory before moving on to harder problems.

Reference excerpt

SDSS J092048.27+302818.3 also known as OGC 330 and SHELS J140.2012763+30.4717820 is a elliptical galaxy located in the constellation of Cancer. The redshift of the galaxy is (z) 0.288. SDSS J092048.27+302818.3 is a massive elliptical galaxy of Type E morphology, residing as the brightest cluster galaxy of the GMBCG J140.20117+30.47176 galaxy cluster. The total R-band magnitude of the galaxy has been estimated to be 16.903 ± 0.001 while its total stellar mass is calculated to be 11.89+0.06−0.08 M☉. The total half-light radius of the galaxy has been estimated to be 2.7396 ± 0.0058 or 4.25 arcseconds while the axial ratios is calculated to be 0.9278 ± 0.0009. Evidence also found it is an early-type galaxy shown lensing an emission-line galaxy located in the background with a redshift of (z) 0.3918. The stellar velocity dispersion of the galaxy itself is 297 ± 17 kilometers per seconds while the major axis position angle of the galaxy is 30°. The total AB magnitude is 16.25. A study published in 2022 has recalculated the stellar mass of the galaxy as 11.786+0.092−0.120 M☉.

References

External links SDSS J092048.27+302818.3 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images

Illustrations

SDSS J092048.27+302818.3 illustration

Worked examples

Example 1 — a first encounter with SDSS J092048.27+302818.3

Start with the simplest possible case. Write down what SDSS J092048.27+302818.3 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 SDSS J092048.27+302818.3 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 SDSS J092048.27+302818.3 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 SDSS J092048.27+302818.3

In research
SDSS J092048.27+302818.3 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 SDSS J092048.27+302818.3 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
SDSS J092048.27+302818.3 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Cancer (constellation), Elliptical galaxies, Gravitational lensing, so understanding it makes those chapters shorter.
In everyday life
Look for SDSS J092048.27+302818.3 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 SDSS J092048.27+302818.3 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what SDSS J092048.27+302818.3 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 SDSS J092048.27+302818.3 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is SDSS J092048.27+302818.3 in simple terms?

SDSS J092048.27+302818.3 also known as OGC 330 and SHELS J140.2012763+30.4717820 is a elliptical galaxy located in the constellation of Cancer. The redshift of the galaxy is (z) 0.288.

Why does SDSS J092048.27+302818.3 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 SDSS J092048.27+302818.3?

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 SDSS J092048.27+302818.3.

Tags

  • Cancer (constellation)
  • Elliptical galaxies
  • Gravitational lensing
  • LEDA objects
  • SDSS objects

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