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astronomy

PKS 1127−145

PKS 1127−145 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 PKS 1127−145 rather than just read about it. In short: PKS 1127−145 is a radio-loud quasar located in the constellation of Crater. This is a Gigahertz Peaked Spectrum object with a redshift of (z) 1.187, first discovered by astronomers in 1966.

PKS 1127−145 — main illustration
PKS 1127−145 — illustration

Key takeaways

  • PKS 1127−145 belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect PKS 1127−145 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of PKS 1127−145 from memory before moving on to harder problems.

Reference excerpt

PKS 1127−145 is a radio-loud quasar located in the constellation of Crater. This is a Gigahertz Peaked Spectrum object with a redshift of (z) 1.187, first discovered by astronomers in 1966. Its radio spectrum appears to be flat making it a flat-spectrum radio quasar, or an FSRQ in short.

Description PKS 1127−145 displays blazar-like behavior. It is known to undergo a period of gamma ray activity, especially in December 2020 where its daily gamma ray flux reached a peak of (E > 100 MeV) of (1.6 ± 0.3) × 10−6 photons cm−2 s−1. Two flares were detected by Fermi-LAT in May and October 2022. The radio structure of PKS 1127−145 is found to be complex. A radio image made by the Very Long Baseline Interferometry (VLBI) shows the object has two components, mainly a bright component and a much weaker component with same brightness temperatures of 1.3 × 1011 Kelvin. No extension is found in northwest direction. There is a presence of a compact core displaying strong increase of flux density with the outermost component being separated into several smaller regions enveloped completely by emission. A stationary feature is also seen located 4 mas from the core via a 22 GHz image taken by VLBI. Circular polarization has also been found in the quasar as well.

X-ray jet

An X-ray jet has been discovered in PKS 1127−145 by Chandra X-ray Observatory. With an estimated length of 300 kiloparsecs, this makes it the longest detected so far in any high redshift quasar. Advanced CCD Imaging Spectrometer also revealed a complex structure in the X-ray jet from the core with bright knots of different morphologies. Two of the knots showed changes in their profiles while the other knot is fainter with presence of X-ray emission scattered over a large area. A more in-depth analysis of the X-ray jet in PKS 1127−145 showed the inner jet of PKS 1127−145 located from the core is found to be extremely polarized and a parallel magnetic field towards the jet's axis. Upon reaching 18 arcseconds from the core, the jet suddenly bends slightly causing the re-brightening of radio emission. In additional, there is a 90° rotation of the magnetic field suggesting it might be compressed to the plane that is found perpendicular to the axis.

References

External links PKS 1127−145 PKS 1127−145 on NASA/IPAC Database

Illustrations

PKS 1127−145 illustration
PKS 1127−145: Chandra image of the X-ray jet in PKS 1127−145
Chandra image of the X-ray jet in PKS 1127−145

Worked examples

Example 1 — a first encounter with PKS 1127−145

Start with the simplest possible case. Write down what PKS 1127−145 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 PKS 1127−145 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 PKS 1127−145 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 PKS 1127−145

In research
PKS 1127−145 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 PKS 1127−145 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
PKS 1127−145 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Active galaxies, Astronomical objects discovered in 1966, Blazars, so understanding it makes those chapters shorter.
In everyday life
Look for PKS 1127−145 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 PKS 1127−145 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what PKS 1127−145 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 PKS 1127−145 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is PKS 1127−145 in simple terms?

PKS 1127−145 is a radio-loud quasar located in the constellation of Crater. This is a Gigahertz Peaked Spectrum object with a redshift of (z) 1.187, first discovered by astronomers in 1966.

Why does PKS 1127−145 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 PKS 1127−145?

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 PKS 1127−145.

Tags

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

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