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QSO B1422+202

QSO B1422+202 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 B1422+202 rather than just read about it. In short: QSO B1422+202 is a quasar located in the constellation of Boötes. The redshift of the object is (z) 0.871.

QSO B1422+202 — main illustration
QSO B1422+202 — illustration

Key takeaways

  • QSO B1422+202 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 B1422+202 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of QSO B1422+202 from memory before moving on to harder problems.

Reference excerpt

QSO B1422+202 is a quasar located in the constellation of Boötes. The redshift of the object is (z) 0.871. It was first discovered by astronomers in 1966 through spectroscopic observations and is designated as 4C 20.33 in the Fourth Cambridge Survey.

Description QSO B1422+202 has a compact steep spectrum source (CSS). When viewed with Very Large Array (VLA) polarimetry imaging, it has a radio core with low polarization and with a lengthy one-sided jet to the south, displaying a large amount of polarized radio emission in its jet components, estimated between 30% and 60%. The jet also shown to be curved as well despite VLA describing it as straight. The structure appears to be bent at its southern end. A radio lobe on the counter-jet side is present in the structure, described as less polarized too with diffused emission located near its nucleus. VLA radio mapping also described the structure of the source as elongated with a faint off-axis region. Additionally, a compact component marked as the beginning of the jet, was found to display an inverted spectral index. Observations made by Very Long Baseline Interferometry (VLBI) at 92 centimeters described the source as diffused instead with emission being concentrated in a 400 milliarcseconds area. More detailed radio imaging made by both VLA and VLBI shows the quasar displaying radio emission blobs in its elongated structure in a north to south direction. There is the same lengthy jet from the previous observations present, pointing towards the direction of south but there is possibly helical shaped based on the components placed along the major axis position angle. Two hotspot features, mainly a weak hotspot and a bright hotspot located in the jet end on opposite side of another component were discovered. The core contains a gigahertz peaked radio spectrum with emission peaking at 4 GHz. The quasar is surrounded by extended ionized emission-line gas according to observations made by William Herschel Telescope (WHT) using a faint object spectrograph. When observed, the gas density is estimated to be 55 cm−3 with a separation gap of 24 kiloparsecs. The oxygen line ratios are similar to the quasar 3C 48 at a low redshift, suggesting it has a high amount of gas density.

References

External links QSO B1422+202 on SIMBAD

Illustrations

QSO B1422+202 illustration

Worked examples

Example 1 — a first encounter with QSO B1422+202

Start with the simplest possible case. Write down what QSO B1422+202 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 B1422+202 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 B1422+202 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 B1422+202

In research
QSO B1422+202 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 B1422+202 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 B1422+202 is common in secondary-school and first-year university syllabi. It links to neighbouring topics 4C objects, Active galaxies, Astronomical objects discovered in 1966, so understanding it makes those chapters shorter.
In everyday life
Look for QSO B1422+202 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 B1422+202 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what QSO B1422+202 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 B1422+202 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is QSO B1422+202 in simple terms?

QSO B1422+202 is a quasar located in the constellation of Boötes. The redshift of the object is (z) 0.871.

Why does QSO B1422+202 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 B1422+202?

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 B1422+202.

Tags

  • 4C objects
  • Active galaxies
  • Astronomical objects discovered in 1966
  • Boötes
  • LEDA objects
  • Quasars
  • ROSAT objects

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