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astronomy

HD 118285

HD 118285 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 118285 rather than just read about it. In short: HD 118285, also known as HR 5115, is a variable star located in the southern circumpolar constellation Chamaeleon. DY Chamaeleontis (DY Cha) is its variable star designation.

HD 118285 — main illustration
HD 118285 — illustration

Key takeaways

  • HD 118285 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 118285 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of HD 118285 from memory before moving on to harder problems.

Reference excerpt

HD 118285, also known as HR 5115, is a variable star located in the southern circumpolar constellation Chamaeleon. DY Chamaeleontis (DY Cha) is its variable star designation. It has an average apparent magnitude of 6.32, placing it near the limit for naked eye visibility. The object is located relatively far at a distance of 864 light years based on Gaia DR3 parallax measurements but is receding with a heliocentric radial velocity of 18 km/s. At its current distance, HD 118285's brightness is diminished by 0.58 magnitudes due to interstellar dust. HD 118285's variability was first observed in a 1998 Hipparcos survey focusing on the discovery of slowly pulsating B-type stars (SPB). It was later confirmed to be an SPB star and given the variable designation DY Chamaeleontis. It fluctuates between magnitudes 6.34 and 6.38 in the visual passband with a period of 23 hours. This is a slightly evolved B-type star with a stellar classification of B8 IV. Contrary to the classification, stellar evolution models from Zorec and Royer (2012) model it as a dwarf star that has completed 89.1% of its main sequence life. It has 3.6 times the mass of the Sun and 5.5 times its girth. It radiates 293 times the luminosity of the Sun from its photosphere at an effective temperature of 11,350 K, giving it a bluish-white hue. It is estimated to be 309 million years old and spins modestly with a projected rotational velocity of 67 km/s.

References

Illustrations

HD 118285 illustration

Worked examples

Example 1 — a first encounter with HD 118285

Start with the simplest possible case. Write down what HD 118285 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 118285 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 118285 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 118285

In research
HD 118285 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 118285 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 118285 is common in secondary-school and first-year university syllabi. It links to neighbouring topics B-type subgiants, Bright Star Catalogue objects, Chamaeleon, so understanding it makes those chapters shorter.
In everyday life
Look for HD 118285 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 118285 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what HD 118285 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 118285 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is HD 118285 in simple terms?

HD 118285, also known as HR 5115, is a variable star located in the southern circumpolar constellation Chamaeleon. DY Chamaeleontis (DY Cha) is its variable star designation.

Why does HD 118285 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 118285?

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 118285.

Tags

  • B-type subgiants
  • Bright Star Catalogue objects
  • Chamaeleon
  • Durchmusterung objects
  • Gould objects
  • Henry Draper Catalogue objects
  • Hipparcos objects
  • Objects with variable star designations
  • Slowly pulsating B-type stars

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