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Gaia BH3

Gaia BH3 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 Gaia BH3 rather than just read about it. In short: Gaia BH3 (Gaia DR3 4318465066420528000) is a binary system consisting of a metal-poor giant star with spectral type G and a stellar-mass black hole. Gaia BH3 is located 1926 light years away (590.6±5.8 pc away) in the constellation of Aquila.

Gaia BH3 — main illustration
Gaia BH3 — illustration

Key takeaways

  • Gaia BH3 belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect Gaia BH3 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of Gaia BH3 from memory before moving on to harder problems.

Reference excerpt

Gaia BH3 (Gaia DR3 4318465066420528000) is a binary system consisting of a metal-poor giant star with spectral type G and a stellar-mass black hole. Gaia BH3 is located 1926 light years away (590.6±5.8 pc away) in the constellation of Aquila. Gaia BH3 is the first black hole discovered from preliminary Gaia DR4 astrometric data. The black hole and star orbit the system barycentre every 11.6 years, with an orbital distance ranging from 4.5–29 AU. The black hole's mass is 32.70 M☉, the most massive known stellar black hole in the Milky Way. The black hole Gaia BH3 is the second known stellar black hole more massive than about 10 M☉ (with the first being Cygnus X-1). The mass of Gaia BH3 is quite similar to the mass of merging binary black holes found via gravitational waves. These massive black holes were suspected to be formed by metal-poor stars and the fact that Gaia BH3 has a metal-poor companion strengthens this conclusion. Gaia BH3 was found to be part of a disrupted star cluster of low mass and this star cluster is today a halo stellar stream, called ED-2. This stellar stream is very old, with an age comparable to the globular cluster Messier 92. This means that Gaia BH3 likely formed more than 13 billion years ago and the black hole might have formed via direct collapse of a massive star. Alternatively the black hole could have formed via binary interaction inside the star cluster. The ED-2 star cluster has a mass between 2,000 M☉ and 42,000 M☉.

Discovery Gaia BH3 was identified in astrometric observations with Gaia, during an analysis in preparation for Data Release 4. It was announced with the publication of a scientific paper in the journal Astronomy & Astrophysics on 16 April 2024.

See also List of nearest known black holes Gaia BH1 Gaia BH2

References

Illustrations

Gaia BH3 illustration

Worked examples

Example 1 — a first encounter with Gaia BH3

Start with the simplest possible case. Write down what Gaia BH3 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 Gaia BH3 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 Gaia BH3 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 Gaia BH3

In research
Gaia BH3 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 Gaia BH3 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
Gaia BH3 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Aquila (constellation), Astrometric binaries, Astronomical objects discovered in 2024, so understanding it makes those chapters shorter.
In everyday life
Look for Gaia BH3 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 Gaia BH3 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what Gaia BH3 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 Gaia BH3 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Gaia BH3 in simple terms?

Gaia BH3 (Gaia DR3 4318465066420528000) is a binary system consisting of a metal-poor giant star with spectral type G and a stellar-mass black hole. Gaia BH3 is located 1926 light years away (590.6±5.8 pc away) in the constellation of Aquila.

Why does Gaia BH3 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 Gaia BH3?

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 Gaia BH3.

Tags

  • Aquila (constellation)
  • Astrometric binaries
  • Astronomical objects discovered in 2024
  • G-type main-sequence stars
  • Population II stars
  • Stellar black holes

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