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HD 101584

HD 101584 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 101584 rather than just read about it. In short: HD 101584 is a suspected post-common envelope binary about 1,800 to 5,900 light-years distant in the constellation of Centaurus. The system is bright at optical wavelengths with an apparent visual magnitude of about 7.

HD 101584 — main illustration
HD 101584 — illustration

Key takeaways

  • HD 101584 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 101584 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of HD 101584 from memory before moving on to harder problems.

Reference excerpt

HD 101584 is a suspected post-common envelope binary about 1,800 to 5,900 light-years distant in the constellation of Centaurus. The system is bright at optical wavelengths with an apparent visual magnitude of about 7. The primary is either a post-AGB star, but more likely a post-RGB star. The secondary is a red dwarf or possibly a low-luminosity white dwarf, which orbits the primary every 150-200 days. The system is surrounded by a slowly rotating circumbinary disk, probably with a face-on orientation towards the Solar System and a size of about 150 astronomical units.

Variability

In 1991, Jean Manfroid et al. published photometry that showed that HD 101584 is a variable star. HD 101584 has been given the variable star designation V885 Centauri. The International Variable Star Index states that the star varies between visual magnitude 6.90 and 7.02, over a period of 87.9 days. However Koen and Eyer detected, in the star's Hipparcos data, an oscillation of the star's brightness with a period of 6.744 days and an amplitude of only 0.02 magnitudes.

Nebula

The Hubble Space Telescope image shows a diffuse circumstellar environment with a circular ring around HD 101584. ALMA mapped the nebula around HD 101584 and was able to map the region close to the central binary. The nebula consists of a central compact source, an equatorial density enhancement (disk), a high-velocity bipolar outflow and an hourglass structure surrounding the outflow. The outflow reaches a maximum velocity of about 150 km/s and is inclined to the line of sight by 10+10−5°. There is evidence for a second bipolar outflow with a different orientation from the major outflow. The inner disk, heated to 1540 K, currently has been sublimated by the increasing luminosity of the star.

Evolution The companion of this system was captured a few hundred years ago, for example when the red giant reached its critical size. It spiralled towards the red giant but stopped before it merged with the core of the primary. During this stage the outer layers of the red giant were ejected. During the common envelope phase the red giant phase of the primary was terminated and the core was revealed. Later, the bipolar jets formed and met the ejected material, forming the hourglass-shaped structure. Ejected material shows prominent spectral features of magnesium, while outer ejected structures contain methanol and formaldehyde.

References

Illustrations

HD 101584 illustration
HD 101584: A light curve for V885 Centauri, plotted from Hipparcos data[6]
A light curve for V885 Centauri, plotted from Hipparcos data[6]
HD 101584: HD 101584 and the surrounding nebula, seen by Hubble
HD 101584 and the surrounding nebula, seen by Hubble

Worked examples

Example 1 — a first encounter with HD 101584

Start with the simplest possible case. Write down what HD 101584 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 101584 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 101584 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 101584

In research
HD 101584 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 101584 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 101584 is common in secondary-school and first-year university syllabi. It links to neighbouring topics A-type supergiants, Binary stars, Centaurus, so understanding it makes those chapters shorter.
In everyday life
Look for HD 101584 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 101584 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what HD 101584 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 101584 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is HD 101584 in simple terms?

HD 101584 is a suspected post-common envelope binary about 1,800 to 5,900 light-years distant in the constellation of Centaurus. The system is bright at optical wavelengths with an apparent visual magnitude of about 7.

Why does HD 101584 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 101584?

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 101584.

Tags

  • A-type supergiants
  • Binary stars
  • Centaurus
  • Henry Draper Catalogue objects
  • Hipparcos objects
  • IRAS catalogue objects
  • Objects with variable star designations
  • Protoplanetary nebulae
  • Variable stars

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