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GSC 02652-01324

GSC 02652-01324 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 GSC 02652-01324 rather than just read about it. In short: GSC 02652-01324, also known as V672 Lyrae, is an orange dwarf main sequence star approximately 521 light-years away in the constellation of Lyra (the Lyre). It hosts one known exoplanet, TrES-1b.

GSC 02652-01324 — main illustration
GSC 02652-01324 — illustration

Key takeaways

  • GSC 02652-01324 belongs to astronomy; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect GSC 02652-01324 to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of GSC 02652-01324 from memory before moving on to harder problems.

Reference excerpt

GSC 02652-01324, also known as V672 Lyrae, is an orange dwarf main sequence star approximately 521 light-years away in the constellation of Lyra (the Lyre). It hosts one known exoplanet, TrES-1b. There is a small, cool companion star at a separation of 13.2 arcseconds, corresponding to 2111 AU.

Nomenclature The designation GSC 02652-01324 comes from the Guide Star Catalog. The star is sometimes called TrES-1, in reference to its planet discovered by the Trans-Atlantic Exoplanet Survey (TrES). The discovery paper and the SIMBAD database use this designation for the planet itself, but other sources call the star TrES-1 and the planet TrES-1b, following the standard exoplanet naming convention. Since the planet transits the star, the star is classified as a planetary transit variable and has received the variable star designation V672 Lyrae. The transits last a little over an hour, about 4% of the orbital period, and the brightness diminishes by a few hundredths of a magnitude.

Planetary system In 2004, the exoplanet TrES-1b was found to be orbiting this star by the Trans-Atlantic Exoplanet Survey using the transit method. The planet was detected crossing its parent star using a small 4-inch-diameter (100 mm) telescope. The discovery was confirmed by the Keck Observatory using the radial velocity method, allowing its mass to be determined. The planet is a hot Jupiter, with a mass and size similar to those of Jupiter but an orbital period of only three days. Evidence of a candidate second planet, designated TrES-1c, was found in 2025 by the radial velocity method. If existing, this planet would have a minimum mass about that of Saturn, and an eccentric orbit with a 1,200-day period. An additional planet in the system is suspected due to transit-timing variations (TTVs) of TrES-1b, but has not been detected. For a planet causing the observed TTVs to remain undetected, it would need to have a mass less than ~0.25 MJ and an orbital period less than ~7 days. Other than the TTVs, there is as yet no evidence of such a planet, but the observed TTVs cannot be explained by other known effects.

See also HD 209458 51 Pegasi

References

External links "Planet TRES-1 b". Extrasolar Planets Encyclopaedia. Retrieved 2018-11-28.

Illustrations

GSC 02652-01324 illustration

Worked examples

Example 1 — a first encounter with GSC 02652-01324

Start with the simplest possible case. Write down what GSC 02652-01324 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 GSC 02652-01324 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 GSC 02652-01324 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 GSC 02652-01324

In research
GSC 02652-01324 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 GSC 02652-01324 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
GSC 02652-01324 is common in secondary-school and first-year university syllabi. It links to neighbouring topics K-type main-sequence stars, Lyra, Objects with variable star designations, so understanding it makes those chapters shorter.
In everyday life
Look for GSC 02652-01324 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 GSC 02652-01324 in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what GSC 02652-01324 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 GSC 02652-01324 out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is GSC 02652-01324 in simple terms?

GSC 02652-01324, also known as V672 Lyrae, is an orange dwarf main sequence star approximately 521 light-years away in the constellation of Lyra (the Lyre). It hosts one known exoplanet, TrES-1b.

Why does GSC 02652-01324 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 GSC 02652-01324?

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 GSC 02652-01324.

Tags

  • K-type main-sequence stars
  • Lyra
  • Objects with variable star designations
  • Planetary systems with one confirmed planet
  • Planetary transit variables
  • TESS Objects of Interest

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