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HD 16417 b

HD 16417 b 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 16417 b rather than just read about it. In short: HD 16417 b (also called λ2 Fornacis b) is an extrasolar planet located approximately 83 light years away in the constellation of Fornax, orbiting the 6th magnitude G-type main sequence star HD 16417. This planet has a minimum mass only 7% that of Jupiter, making it a Neptune-mass planet.

HD 16417 b — main illustration
HD 16417 b — illustration

Key takeaways

  • HD 16417 b 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 16417 b to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of HD 16417 b from memory before moving on to harder problems.

Reference excerpt

HD 16417 b (also called λ2 Fornacis b) is an extrasolar planet located approximately 83 light years away in the constellation of Fornax, orbiting the 6th magnitude G-type main sequence star HD 16417. This planet has a minimum mass only 7% that of Jupiter, making it a Neptune-mass planet. In addition to this, it orbits relatively close to the host star and suffers high temperature. It is the third planet discovered in the Fornax constellation on February 23, 2009. This planet was discovered by a method called the radial velocity method.

References

Illustrations

HD 16417 b illustration

Worked examples

Example 1 — a first encounter with HD 16417 b

Start with the simplest possible case. Write down what HD 16417 b 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 16417 b 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 16417 b 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 16417 b

In research
HD 16417 b 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 16417 b 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 16417 b is common in secondary-school and first-year university syllabi. It links to neighbouring topics Exoplanet stubs, Exoplanets detected by radial velocity, Exoplanets discovered in 2009, so understanding it makes those chapters shorter.
In everyday life
Look for HD 16417 b 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 16417 b in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what HD 16417 b 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 16417 b out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is HD 16417 b in simple terms?

HD 16417 b (also called λ2 Fornacis b) is an extrasolar planet located approximately 83 light years away in the constellation of Fornax, orbiting the 6th magnitude G-type main sequence star HD 16417. This planet has a minimum mass only 7% that of Jupiter, making it a Neptune-mass planet.

Why does HD 16417 b 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 16417 b?

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 16417 b.

Tags

  • Exoplanet stubs
  • Exoplanets detected by radial velocity
  • Exoplanets discovered in 2009
  • Fornax
  • Giant planets
  • Hot Neptunes

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