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astronomy

HD 13189

HD 13189 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 HD 13189 rather than just read about it. In short: HD 13189 is a star in the northern constellation of Triangulum constellation. With an apparent visual magnitude of +7.57, it is too faint to be visible to the normal human eye.

HD 13189 — main illustration
HD 13189 — illustration

Key takeaways

  • HD 13189 belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect HD 13189 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of HD 13189 from memory before moving on to harder problems.

Reference excerpt

HD 13189 is a star in the northern constellation of Triangulum constellation. With an apparent visual magnitude of +7.57, it is too faint to be visible to the normal human eye. The distance to this system is approximately 1,590 light years based on parallax measurements, and it is drifting further away with a radial velocity of 25.39 km/s. In 2005, a planetary companion or brown dwarf was announced in orbit around this star. It has a spectral classification of K1II-III, making it a giant star that has evolved away from the main sequence after exhausting the hydrogen at its core. The mass is 1.2 times the Sun's, while measurements of the star's radius give estimates of 38 R☉. The atmosphere of the star displays short period radial velocity variations with a primary period of 4.89 days. This behavior is typical for giant K-type stars such as this and it is not the result of a close-orbit planetary companion.

HD 13189 b

HD 13189 b is an exoplanet or brown dwarf with mass ranges from 8 to 20 Jupiter mass. This object is located at a mean distance of 277 million km (1.85 AU) from the star, taking 472 days to make one elliptical orbit. This object was discovered in Tautenburg, Germany in 2005.

References

External links "HD 13189 -- Star". SIMBAD. Retrieved December 21, 2007. "HD 13189 b -- Extra-solar Planet Candidate". SIMBAD. Retrieved December 21, 2007.

Worked examples

Example 1 — a first encounter with HD 13189

Start with the simplest possible case. Write down what HD 13189 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 HD 13189 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 HD 13189 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 HD 13189

In research
HD 13189 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 HD 13189 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
HD 13189 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Brown dwarfs, Durchmusterung objects, Henry Draper Catalogue objects, so understanding it makes those chapters shorter.
In everyday life
Look for HD 13189 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 HD 13189 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what HD 13189 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 HD 13189 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is HD 13189 in simple terms?

HD 13189 is a star in the northern constellation of Triangulum constellation. With an apparent visual magnitude of +7.57, it is too faint to be visible to the normal human eye.

Why does HD 13189 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 HD 13189?

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 HD 13189.

Tags

  • Brown dwarfs
  • Durchmusterung objects
  • Henry Draper Catalogue objects
  • Hipparcos objects
  • K-type bright giants
  • K-type giants
  • Planetary systems with one confirmed planet
  • Triangulum

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