ArticleslgStudy

astronomy

PKS 1502+036

PKS 1502+036 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 1502+036 rather than just read about it. In short: PKS 1502+036 is a narrow-line Seyfert galaxy located in the constellation of Virgo. The redshift of the object has been estimated as (z) 0.408 and it was first discovered as a quasar with a flat radio spectrum by astronomers in 1997.

PKS 1502+036 — main illustration
PKS 1502+036 — illustration

Key takeaways

  • PKS 1502+036 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 1502+036 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of PKS 1502+036 from memory before moving on to harder problems.

Reference excerpt

PKS 1502+036 is a narrow-line Seyfert galaxy located in the constellation of Virgo. The redshift of the object has been estimated as (z) 0.408 and it was first discovered as a quasar with a flat radio spectrum by astronomers in 1997. It is described as radio-loud.

Description PKS 1502+036 is shown to be a gamma-ray emitting object, with one powerful flare displayed in late 2015 after a long period of low-activity with a measured low flux of 4.5×10−8 photon cm−2 s−1. By the time the flare reached a daily peak flux on December 20, 2015, the source had an estimated flux of (237±71)×10−8 photon cm−2 s−1 on a three-hour timescale which in turn, corresponds to a measured isotropic luminosity of (7.3±2.1)×1047 erg s−1. No signs of spectral changes were accompanying the flare, although an increase in optical, ultraviolet and X-ray activity was noted for the object. During intra-night optical monitoring, the source displayed short-term optical variability between April 21 and May 11, 2018, with a brightness change of 0.1 magnitude. The source of PKS 1502+036 is classified as compact double. When imaged with Very Long Baseline Array (VLBA) at 15 GHz, it has an extended radio structure indicative of a core-jet morphology, with radio emission being dominated by a compact radio core that is shown having low fractional polarization and a weak jet-like feature extending out by three milliarcseconds. A weak component with a separation of 3.05 milliarcseconds from its core, appears present in the source which was found undetected through previous observations. The radio spectrum of the source is classified as inverted. Near-infrared imaging obtained by Very Large Telescope, found PKS 1502+036 is an elliptical galaxy based on its surface brightness profile described by a combination of bulge and a nuclear component modelling. There is also a presence of an extended structure in a form of bright spots with position angles between 270 and 370 degrees indicative of galaxy mergers. On the other side of the galaxy center, a more dim extended bar-like structure is seen going from east-southeast to north direction. The supermassive black hole mass for the galaxy has been estimated as7×108 M☉ based on its near-infrared bulge luminosity. There is a close companion near the galaxy, however it isn't interacting with it.

References

External links PKS 1502+036 on WikiSky: DSS2, SDSS, GALEX, IRAS, Hydrogen α, X-Ray, Astrophoto, Sky Map, Articles and images PKS 1502+036 on SIMBAD PKS 1502+036 on HyperLeda

Illustrations

PKS 1502+036 illustration

Worked examples

Example 1 — a first encounter with PKS 1502+036

Start with the simplest possible case. Write down what PKS 1502+036 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 1502+036 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 1502+036 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 1502+036

In research
PKS 1502+036 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 1502+036 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 1502+036 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Active galaxies, Astronomical objects discovered in 1997, Principal Galaxies Catalogue objects, so understanding it makes those chapters shorter.
In everyday life
Look for PKS 1502+036 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.
Ask Teacher Smith questions about this articleOpens your AI tutor with a question about “PKS 1502+036” →

Affiliate

Preply — study more efficiently by working with a personal tutor. 50% off.

How to study PKS 1502+036 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what PKS 1502+036 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 1502+036 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is PKS 1502+036 in simple terms?

PKS 1502+036 is a narrow-line Seyfert galaxy located in the constellation of Virgo. The redshift of the object has been estimated as (z) 0.408 and it was first discovered as a quasar with a flat radio spectrum by astronomers in 1997.

Why does PKS 1502+036 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 1502+036?

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 1502+036.

Tags

  • Active galaxies
  • Astronomical objects discovered in 1997
  • Principal Galaxies Catalogue objects
  • Quasars
  • SDSS objects
  • Seyfert galaxies
  • Virgo (constellation)

Keep exploring