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astronomy

HD 84117

HD 84117 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 84117 rather than just read about it. In short: HD 84117 is a star in the constellation of Hydra. It has an apparent visual magnitude of 4.92, hence can be seen from the naked eye in sufficiently dark skies, far from light pollution.

HD 84117 — main illustration
HD 84117 — illustration

Key takeaways

  • HD 84117 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 84117 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of HD 84117 from memory before moving on to harder problems.

Reference excerpt

HD 84117 is a star in the constellation of Hydra. It has an apparent visual magnitude of 4.92, hence can be seen from the naked eye in sufficiently dark skies, far from light pollution. Based on parallax measurements, it lies 48.77 light-years away. It is drifting away from the Solar System at a radial velocity of 34.7 km/s. With a spectral class of F8V, this is a F star which is in the main sequence, fusing atoms of hydrogen into helium. Stellar evolution models suggest it is approaching the end of its main sequence lifetime. The star has about 1.15 times the Sun's mass and 1.30 times the Sun's radius. It radiates 2.05 times the Sun's luminosity from the photosphere at an effective temperature of 6,229 K. Its age is estimated at 2.6 billion years. This star has a cold debris disk with a radius of 27.27 astronomical units. The temperature of the debris is estimated at 60 K (−213.2 °C), and the total mass of the disk is estimated at 1.2×10−5 Earth masses. Unlike other debris disk hosts, HD 84117 does not display an infrared excess. The disk contributes to less than 1.7%×10−4 of the system's luminosity. HD 84117 presents a significant difference on proper motion measurements taken by the Hipparcos and Gaia spacecraft, suggesting it may be orbited by a giant planet.

See also List of nearest F-type stars

References

Illustrations

HD 84117 illustration

Worked examples

Example 1 — a first encounter with HD 84117

Start with the simplest possible case. Write down what HD 84117 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 84117 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 84117 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 84117

In research
HD 84117 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 84117 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 84117 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Bright Star Catalogue objects, Durchmusterung objects, F-type main-sequence stars, so understanding it makes those chapters shorter.
In everyday life
Look for HD 84117 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 84117 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what HD 84117 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 84117 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is HD 84117 in simple terms?

HD 84117 is a star in the constellation of Hydra. It has an apparent visual magnitude of 4.92, hence can be seen from the naked eye in sufficiently dark skies, far from light pollution.

Why does HD 84117 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 84117?

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 84117.

Tags

  • Bright Star Catalogue objects
  • Durchmusterung objects
  • F-type main-sequence stars
  • Gliese and GJ objects
  • Henry Draper Catalogue objects
  • Hipparcos objects
  • Hydra (constellation)
  • Solar analogs

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