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Königstuhl 1

Königstuhl 1 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 Königstuhl 1 rather than just read about it. In short: Königstuhl 1 (KO-1, Kö 1, Koenigstuhl 1) is a binary consisting out of the red dwarf LEHPM 494 and the M- or L-type star or brown dwarf DENIS-P J0021.0-4244. While similar low-mass wide binary were known in young star-forming regions, Königstuhl1 was the first wide binary detected in the field and was not associated with a star-forming region.

Königstuhl 1 — main illustration
Königstuhl 1 — illustration

Key takeaways

  • Königstuhl 1 belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect Königstuhl 1 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of Königstuhl 1 from memory before moving on to harder problems.

Reference excerpt

Königstuhl 1 (KO-1, Kö 1, Koenigstuhl 1) is a binary consisting out of the red dwarf LEHPM 494 and the M- or L-type star or brown dwarf DENIS-P J0021.0-4244. While similar low-mass wide binary were known in young star-forming regions, Königstuhl1 was the first wide binary detected in the field and was not associated with a star-forming region.

Name and discovery The individual components were known since 1998 (DENIS survey) and 2003 (LEHPM survey), but the binary status was not noticed until José A. Caballero studied them in 2007 and discovered that they move in the same direction. This similar motion was first revealed in the USNO-B1/NOMAD1 proper motion surveys. Caballero also collected 22 years of data to show that the proper motion is consistent. He named the pair Königstuhl 1 because he worked at the Max Planck Institute for Astronomy, which is located on top of the Königstuhl. Other low-mass binaries were discovered by Caballero in the Koenigstuhl survey and called Koenigstuhl 1, Koenigstuhl 2 (Kö 2, Kö 3). The last addition was Koenigstuhl 7 in 2014.

The binary In the discovery paper Caballero reports a spectral type of M6V for the primary Kö 1A and a mass of around 10% of the sun. The spectral type of the secondary Kö 1B was first estimated to be >M9V and later the optical spectral type was determined to be M9.5V. Caballero determined a mass of 79 to 87 MJ for the secondary. The binary components are separated by around 1800 astronomical units. This wide orbit also meant that the gravitational binding energy is very low for the binary. At this time one theory existed that explained the presence of low-mass stars and brown dwarfs with the fragmentation and ejection of stellar embryos from molecular clouds. The presence of wide binaries in the field are hard to explain by such a scenario. The infrared spectral type of Kö 1B was determined to be L0.6: in 2014. The gravity on this object is consistent with other old field dwarfs. Later it was determined that Kö 1 could be part of the 200 Myr old Carina Near Association. If this is true, Kö 1B would be less massive and it would have a mass of 51.88±3.6 MJ. A more precise separation of 2083.4 AU was reported in 2021 and Kö 1B might have two components.

See also Other low-mass wide binaries:

2MASS J11011926−7732383 WISE 2150−7520 SDSS J141624.08+134826.7 UScoCTIO 108 Oph 162225-240515

References

Illustrations

Königstuhl 1 illustration

Worked examples

Example 1 — a first encounter with Königstuhl 1

Start with the simplest possible case. Write down what Königstuhl 1 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 Königstuhl 1 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 Königstuhl 1 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 Königstuhl 1

In research
Königstuhl 1 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 Königstuhl 1 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
Königstuhl 1 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Binary stars, Brown dwarfs, L-type brown dwarfs, so understanding it makes those chapters shorter.
In everyday life
Look for Königstuhl 1 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 Königstuhl 1 in 20 minutes

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

Frequently asked questions

What is Königstuhl 1 in simple terms?

Königstuhl 1 (KO-1, Kö 1, Koenigstuhl 1) is a binary consisting out of the red dwarf LEHPM 494 and the M- or L-type star or brown dwarf DENIS-P J0021.0-4244. While similar low-mass wide binary were known in young star-forming regions, Königstuhl1 was the first wide binary detected in the field and…

Why does Königstuhl 1 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 Königstuhl 1?

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 Königstuhl 1.

Tags

  • Binary stars
  • Brown dwarfs
  • L-type brown dwarfs
  • M-type pre-main-sequence stars
  • Phoenix (constellation)

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