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HD 131399

HD 131399 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 131399 rather than just read about it. In short: HD 131399 is a star system in the constellation of Centaurus. Based on the system's electromagnetic spectrum, it is located around 350 light-years (107.9 parsecs) away.

HD 131399 — main illustration
HD 131399 — illustration

Key takeaways

  • HD 131399 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 131399 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of HD 131399 from memory before moving on to harder problems.

Reference excerpt

HD 131399 is a star system in the constellation of Centaurus. Based on the system's electromagnetic spectrum, it is located around 350 light-years (107.9 parsecs) away. The total apparent magnitude is 7.07, but because of interstellar dust between it and the Earth, it appears 0.22±0.09 magnitudes dimmer than it should. The brightest star, is a young A-type main-sequence star, and further out are three lower-mass stars. A Jupiter-mass planet or a low-mass brown dwarf was once thought to be orbiting the central star, but this has been ruled out.

Stellar system The brightest star in the HD 131399 system is designated HD 131399 A. Its spectral type is A1V, and it is 2.08 times as massive as the Sun. The two lower-mass stars are designated HD 131399 B and C, respectively. B is a G-type main-sequence star, while HD 131399 C is a K-type main-sequence star. Both stars are less massive than the Sun. A lower-mass companion to HD 131399 A was announced in 2017, at a separation of 0.12 astronomical units (au). HD 131399 B and C are located very close to each other, and the two orbit each other at about 10 AU. In turn, the B-C pair orbits the central star A at a distance of 349 AU. This orbit takes about 3,600 years to complete, and it has an eccentricity of about 0.13 The entire system is about 21.9 million years old. One paper has reported that HD 131399 A has a companion in an inclined 10-day orbit with a semi-major axis of 0.1 AU. HD 131399 A has been described as a "nascent Am star"; although it has a very slow projected rotation rate and would be expected to show chemical peculiarities, its spectrum is relatively normal, possibly due to its young age.

Claims of a planetary system

The claimed discovery of a massive planet, named HD 131399 Ab, was announced in a paper published in the journal Science. The object was imaged using the SPHERE imager of the Very Large Telescope at the European Southern Observatory, located in the Atacama Desert of Chile, and announced in a July 2016 paper in the journal Science. It was thought to be a T-type object with a mass of 4±1 MJ, but its orbit would have been unstable, causing it to be ejected between the primary's red giant phase and white dwarf phase. This was the first exoplanet candidate to be discovered by SPHERE. The image was created from two separate SPHERE observations: one to image the three stars and one to detect the faint planet. After its discovery, the team unofficially named the system "Scorpion-1" and the planet "Scorpion-1b", after the survey that prompted its discovery, the Scorpion Planet Survey (principal investigator: Daniel Apai). In May 2017, observations made by the Gemini Planet Imager and including a reanalysis of the SPHERE data suggest that this target is, in fact, a background star. This object's spectrum seems to be like that of a K-type or M-type dwarf, not a T-type object as first thought. It also initially appeared to be associated with HD 131399, but this was because of its unusually high proper motion (in the top 4% fastest-moving stars). After subsequent data published in 2022 confirmed that the object is a background star, the paper announcing the putative discovery was retracted.

References

Notes

Illustrations

HD 131399 illustration
HD 131399: Artist's impression of HD 131399 Ab, before it was found to be a background star.
Artist's impression of HD 131399 Ab, before it was found to be a background star.

Worked examples

Example 1 — a first encounter with HD 131399

Start with the simplest possible case. Write down what HD 131399 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 131399 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 131399 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 131399

In research
HD 131399 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 131399 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 131399 is common in secondary-school and first-year university syllabi. It links to neighbouring topics A-type main-sequence stars, Centaurus, Durchmusterung objects, so understanding it makes those chapters shorter.
In everyday life
Look for HD 131399 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 131399 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what HD 131399 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 131399 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is HD 131399 in simple terms?

HD 131399 is a star system in the constellation of Centaurus. Based on the system's electromagnetic spectrum, it is located around 350 light-years (107.9 parsecs) away.

Why does HD 131399 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 131399?

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 131399.

Tags

  • A-type main-sequence stars
  • Centaurus
  • Durchmusterung objects
  • G-type main-sequence stars
  • Henry Draper Catalogue objects
  • Hipparcos objects
  • Hypothetical planetary systems
  • K-type main-sequence stars
  • Triple star systems

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