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WISEA J160318.98+031644.8

WISEA J160318.98+031644.8 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 WISEA J160318.98+031644.8 rather than just read about it. In short: WISEA J160318.98+031644.8 also known as OGC 1012, is a radio galaxy located in the constellation of Serpens. The redshift of the galaxy is (z) 0.222 and it was first discovered in a sample of 2,712 radio-loud active galactic nuclei obtained by the Sloan Digital Sky Survey (SDSS) in September 2005.

WISEA J160318.98+031644.8 — main illustration
WISEA J160318.98+031644.8 — illustration

Key takeaways

  • WISEA J160318.98+031644.8 belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect WISEA J160318.98+031644.8 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of WISEA J160318.98+031644.8 from memory before moving on to harder problems.

Reference excerpt

WISEA J160318.98+031644.8 also known as OGC 1012, is a radio galaxy located in the constellation of Serpens. The redshift of the galaxy is (z) 0.222 and it was first discovered in a sample of 2,712 radio-loud active galactic nuclei obtained by the Sloan Digital Sky Survey (SDSS) in September 2005.

Description WISEA J160318.98+031644.8 is a giant elliptical galaxy of type E morphology. It is also a luminous red galaxy found to reside in the center as the brightest cluster galaxy (BCG) of the galaxy cluster, WHL J160319.0+031645 with at least 114 confirmed member candidates. The estimated J-band and H-band infrared color magnitudes of the galaxy is 15.84 and 15.00 magnitudes respectively. The absolute magnitude of the galaxy is -23.42 and it has a total stellar mass of 11.34 M☉. The nucleus is active and has been categorized as a Fanaroff-Riley Class Type II radio galaxy. The radio flux density calculated by the NRAO VLA Sky Survey (NVSS) at 1.4 GHz frequencies is 127.00 mJy. The radio luminosity is 25.26 W Hz−1. A study published in 2022, found it is a bent-tailed radio galaxy which can be further classified as a wide-angle tail radio galaxy. The total flux density estimated at 1.4 GHz is 132.94 mJy, while the flux density at 3 GHz is 66.86 mJy. The spectral index between 1.4 and 3 GHz is 0.9α. A radio jet has been detected, with a jet opening angle of 132.8° and a jet curvature radius of 30.8 arcseconds. The radio lobes are resolved, with a flux density of 0.128 Jy and have lobe to lobe separation by 0.002° while the radio core remains undetected. The largest angular size of the galaxy is 34 arcseconds and the largest linear size is 126.0 kiloparsecs. Evidence also found the source is a double, with an approximate bending angle of 41.3°. The excess bending angle is 34.4°.

References

External links WISEA J160318.98+031644.8 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images WISEA J160318.98+031644.8 on HyperLeda

Illustrations

WISEA J160318.98+031644.8 illustration

Worked examples

Example 1 — a first encounter with WISEA J160318.98+031644.8

Start with the simplest possible case. Write down what WISEA J160318.98+031644.8 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 WISEA J160318.98+031644.8 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 WISEA J160318.98+031644.8 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 WISEA J160318.98+031644.8

In research
WISEA J160318.98+031644.8 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 WISEA J160318.98+031644.8 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
WISEA J160318.98+031644.8 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Active galaxies, Astronomical objects discovered in 2005, Elliptical galaxies, so understanding it makes those chapters shorter.
In everyday life
Look for WISEA J160318.98+031644.8 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 WISEA J160318.98+031644.8 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what WISEA J160318.98+031644.8 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 WISEA J160318.98+031644.8 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is WISEA J160318.98+031644.8 in simple terms?

WISEA J160318.98+031644.8 also known as OGC 1012, is a radio galaxy located in the constellation of Serpens. The redshift of the galaxy is (z) 0.222 and it was first discovered in a sample of 2,712 radio-loud active galactic nuclei obtained by the Sloan Digital Sky Survey (SDSS) in September 2005.

Why does WISEA J160318.98+031644.8 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 WISEA J160318.98+031644.8?

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 WISEA J160318.98+031644.8.

Tags

  • Active galaxies
  • Astronomical objects discovered in 2005
  • Elliptical galaxies
  • LEDA objects
  • Radio galaxies
  • SDSS objects
  • Serpens
  • WISE objects

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