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OGLE-2011-BLG-0462

OGLE-2011-BLG-0462 is a science 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 OGLE-2011-BLG-0462 rather than just read about it. In short: OGLE-2011-BLG-0462, also known as MOA-2011-BLG-191, is a stellar-mass black hole isolated in interstellar space. OGLE-2011-BLG-0462 lies at a distance of 1,720 parsecs (5,610 light years) in the direction of the galactic bulge in the constellation Sagittarius.

OGLE-2011-BLG-0462 — main illustration
OGLE-2011-BLG-0462 — illustration

Key takeaways

  • OGLE-2011-BLG-0462 belongs to science; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect OGLE-2011-BLG-0462 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of OGLE-2011-BLG-0462 from memory before moving on to harder problems.

Reference excerpt

OGLE-2011-BLG-0462, also known as MOA-2011-BLG-191, is a stellar-mass black hole isolated in interstellar space. OGLE-2011-BLG-0462 lies at a distance of 1,720 parsecs (5,610 light years) in the direction of the galactic bulge in the constellation Sagittarius. The black hole has a mass of about 7.15 M☉. OGLE-2011-BLG-0462 is the first truly isolated black hole which has been confirmed.

Discovery OGLE-2011-BLG-0462 was discovered by the OGLE survey through microlensing when it passed in front of a background star that was 20,000 light years away from Earth. The black hole's gravity bent the star's light, causing a sharp spike in brightness that was detected by the Hubble Space Telescope. It took six years to confirm the existence of OGLE-2011-BLG-0462. Its initial kick velocity has been estimated to have an upper limit of 100 km/s. No significant X-ray emission has been detected from gas accreting onto the black hole indicating that it is truly isolated.

References

Illustrations

OGLE-2011-BLG-0462 illustration

Worked examples

Example 1 — a first encounter with OGLE-2011-BLG-0462

Start with the simplest possible case. Write down what OGLE-2011-BLG-0462 claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In science, 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 OGLE-2011-BLG-0462 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 OGLE-2011-BLG-0462 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 OGLE-2011-BLG-0462

In research
OGLE-2011-BLG-0462 appears in science 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 OGLE-2011-BLG-0462 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
OGLE-2011-BLG-0462 is common in secondary-school and first-year university syllabi. It links to neighbouring topics Gravitational lensing, Sagittarius (constellation), Stellar black holes, so understanding it makes those chapters shorter.
In everyday life
Look for OGLE-2011-BLG-0462 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 OGLE-2011-BLG-0462 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what OGLE-2011-BLG-0462 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 OGLE-2011-BLG-0462 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is OGLE-2011-BLG-0462 in simple terms?

OGLE-2011-BLG-0462, also known as MOA-2011-BLG-191, is a stellar-mass black hole isolated in interstellar space. OGLE-2011-BLG-0462 lies at a distance of 1,720 parsecs (5,610 light years) in the direction of the galactic bulge in the constellation Sagittarius.

Why does OGLE-2011-BLG-0462 matter?

Because it connects several science 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 OGLE-2011-BLG-0462?

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 OGLE-2011-BLG-0462.

Tags

  • Gravitational lensing
  • Sagittarius (constellation)
  • Stellar black holes

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