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QSO B1524−136

QSO B1524−136 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 QSO B1524−136 rather than just read about it. In short: QSO B1524−136 is a quasar located in the constellation of Libra. It has a redshift of (z) 1.687 and it was first identified by astronomers from the Parkes Observatory in 1966.

QSO B1524−136 — main illustration
QSO B1524−136 — illustration

Key takeaways

  • QSO B1524−136 belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect QSO B1524−136 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of QSO B1524−136 from memory before moving on to harder problems.

Reference excerpt

QSO B1524−136 is a quasar located in the constellation of Libra. It has a redshift of (z) 1.687 and it was first identified by astronomers from the Parkes Observatory in 1966. The object is classified as a compact steep spectrum source (CSS) and is noted for its two-sided radio jet.

Description QSO B1524−136 is a radio-loud AGN. It has a radio spectrum that appears as steep but also flat. M. Bondi classifies the source as variable at low frequencies although no significant variations in flux density have been detected. The supermassive black hole mass for this object is estimated to be 9.52 M☉ based on assumptions of absorption lines. The radio structure of QSO B1524−136 is quite compact. Observations with Very Long Baseline Interferometry (VLBI) showed, its structure as elongated at 45° while a double structure imaged by Very Large Array A-array showed it as double. When imaged by MERLIN at 5 GHz, the structure has two main components located in north and south directions, with the former having a high peak brightness. A radio image taken by MK2 VLBI, found it having a bright northern hotspot and a jet connecting from the radio core to the hotspot. This jet is estimated to have a width of 7 milliarcseconds and a length of 35 milliarcseconds. A low radio emission gap can also be seen between the core and the jet's start point. Very Long Baseline Array (VLBA) also detected the same jet, displaying a series of knots. They appeared to be bent by 40° before entering the hotspot region. A counter-jet was also detected by VLBA, making QSO B1524−136 having two jets on each side of its nucleus. Polarization has been observed in several jet regions of QSO B1524−136. However its rotation measure value changes as the jet travels from one region to the next. This change might be explained by an external screen whose magnetic field orientation varies along with the jet, in the way rotation measure variations are reproduced. A large rotation measure has been found for its strong northern component, with a value of 20,411 rad m−2.

References

External links QSO B1524−136 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images QSO B1524−136 on SIMBAD

Illustrations

QSO B1524−136 illustration

Worked examples

Example 1 — a first encounter with QSO B1524−136

Start with the simplest possible case. Write down what QSO B1524−136 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 QSO B1524−136 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 QSO B1524−136 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 QSO B1524−136

In research
QSO B1524−136 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 QSO B1524−136 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
QSO B1524−136 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Active galaxies, Astronomical objects discovered in 1966, LEDA objects, so understanding it makes those chapters shorter.
In everyday life
Look for QSO B1524−136 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 QSO B1524−136 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what QSO B1524−136 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 QSO B1524−136 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is QSO B1524−136 in simple terms?

QSO B1524−136 is a quasar located in the constellation of Libra. It has a redshift of (z) 1.687 and it was first identified by astronomers from the Parkes Observatory in 1966.

Why does QSO B1524−136 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 QSO B1524−136?

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 QSO B1524−136.

Tags

  • Active galaxies
  • Astronomical objects discovered in 1966
  • LEDA objects
  • Libra (constellation)
  • Quasars

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