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HD 102195 b

HD 102195 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 102195 b rather than just read about it. In short: HD 102195 b (also called ET-1, and formally named Lete) is an extrasolar planet orbiting the star HD 102195 in the constellation of Virgo, discovered in January 2006. It is the first planet discovered by the Exoplanet Tracker project, using a dispersed fixed-delay interferometer.

Key takeaways

  • HD 102195 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 102195 b to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of HD 102195 b from memory before moving on to harder problems.

Reference excerpt

HD 102195 b (also called ET-1, and formally named Lete) is an extrasolar planet orbiting the star HD 102195 in the constellation of Virgo, discovered in January 2006. It is the first planet discovered by the Exoplanet Tracker project, using a dispersed fixed-delay interferometer. It was discovered at the Kitt Peak National Observatory. The planet is an example of a hot Jupiter, and is likely to be a gas giant based on its mass. The planet HD 102195 b is named Lete. The name was selected in the NameExoWorlds campaign by Italy, during the 100th anniversary of the IAU. Lete is the oblivion river made of fog from Greek mythology in the Italian narrative poem on the afterlife Divina Commedia.

References

External links "HD 102195". Exoplanets. Archived from the original on 2009-11-25. Retrieved 2008-11-04.

Worked examples

Example 1 — a first encounter with HD 102195 b

Start with the simplest possible case. Write down what HD 102195 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 102195 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 102195 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 102195 b

In research
HD 102195 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 102195 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 102195 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 2006, so understanding it makes those chapters shorter.
In everyday life
Look for HD 102195 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 102195 b in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what HD 102195 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 102195 b out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is HD 102195 b in simple terms?

HD 102195 b (also called ET-1, and formally named Lete) is an extrasolar planet orbiting the star HD 102195 in the constellation of Virgo, discovered in January 2006. It is the first planet discovered by the Exoplanet Tracker project, using a dispersed fixed-delay interferometer.

Why does HD 102195 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 102195 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 102195 b.

Tags

  • Exoplanet stubs
  • Exoplanets detected by radial velocity
  • Exoplanets discovered in 2006
  • Exoplanets with proper names
  • Giant planets
  • Hot Jupiters
  • Virgo (constellation)

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