astronomy

GSC 06214-00210 b

GSC 06214-00210 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 GSC 06214-00210 b rather than just read about it. In short: GSC 06214-00210 b is a gas giant exoplanet orbiting the K-type star GSC 06214-00210 which is located approximately 356 light-years from Earth in the constellation Scorpius. Discovery GSC 06214-00210 b, along with 1RXS J160929.1−210524 b, was first reported in 2010 as part of an adaptive optics imaging survey targeting wide companions (~50–500 AU) to solar-type stars in the Upper Scorpius association.

Key takeaways

GSC 06214-00210 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 GSC 06214-00210 b to a quantity you can measure, compute or draw — that is where exam questions come from.
Reproduce the core statement of GSC 06214-00210 b from memory before moving on to harder problems.

Reference excerpt

GSC 06214-00210 b is a gas giant exoplanet orbiting the K-type star GSC 06214-00210 which is located approximately 356 light-years from Earth in the constellation Scorpius.

Discovery GSC 06214-00210 b, along with 1RXS J160929.1−210524 b, was first reported in 2010 as part of an adaptive optics imaging survey targeting wide companions (~50–500 AU) to solar-type stars in the Upper Scorpius association. The discovery paper, published in 2011, identified it as a ~14 Jupiter-mass companion and confirmed its comoving status with the host star. Follow-up spectroscopy observations in the same year refined its properties and also the spectral type of L0±1, with multiple signs of youth.

Characteristics Near-infrared spectroscopy revealed exceptionally strong Paschen β emission (equivalent width −11.4 ± 0.3 Å), indicating the presence of a circumplanetary accretion disk. Subsequent studies have documented variability in the H I Paschen β emission line on timescales from minutes to decades, with moderate flux changes (<50%) on short scales and larger variations (up to ~1000%) over years, resembling classical T Tauri stars. There are line profiles for GSC 06214-00210 b and GQ Lupi b, and for GSC 06214-00210 b, they are consistent with both magnetospheric accretion and shock models, though shock models are favored in the brightest epochs.

See also List of directly imaged exoplanets

References

Illustrations

Worked examples

Example 1 — a first encounter with GSC 06214-00210 b

Start with the simplest possible case. Write down what GSC 06214-00210 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 GSC 06214-00210 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 GSC 06214-00210 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 GSC 06214-00210 b

In research: GSC 06214-00210 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 GSC 06214-00210 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: GSC 06214-00210 b is common in secondary-school and first-year university syllabi. It links to neighbouring topics Exoplanets detected by direct imaging, Exoplanets discovered in 2010, so understanding it makes those chapters shorter.
In everyday life: Look for GSC 06214-00210 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 GSC 06214-00210 b in 20 minutes

Read the reference excerpt below once, without taking notes.
Close the page and write down what GSC 06214-00210 b means in your own words.
Compare your version with the excerpt and mark what you missed.
Work through the three examples above with pen and paper.
Explain GSC 06214-00210 b out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is GSC 06214-00210 b in simple terms?

GSC 06214-00210 b is a gas giant exoplanet orbiting the K-type star GSC 06214-00210 which is located approximately 356 light-years from Earth in the constellation Scorpius. Discovery GSC 06214-00210 b, along with 1RXS J160929.1−210524 b, was first reported in 2010 as part of an adaptive optics imag…

Why does GSC 06214-00210 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 GSC 06214-00210 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 GSC 06214-00210 b.