astronomy

Gliese 357 d

Gliese 357 d 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 Gliese 357 d rather than just read about it. In short: GJ 357 d is an exoplanet, considered to be a super-Earth within the habitable zone of its parent star. The planet orbits GJ 357, 31 light-years from Earth, The system is part of the Hydra constellation.

Key takeaways

Gliese 357 d belongs to astronomy; place it in that map before memorising details.
Learn the definition first, then one example that makes the definition concrete.
Connect Gliese 357 d to a quantity you can measure, compute or draw — that is where exam questions come from.
Reproduce the core statement of Gliese 357 d from memory before moving on to harder problems.

Reference excerpt

GJ 357 d is an exoplanet, considered to be a super-Earth within the habitable zone of its parent star. The planet orbits GJ 357, 31 light-years from Earth, The system is part of the Hydra constellation. The planet was discovered by the TESS team and announced in July 2019. The data confirming the presence of the planet was uncovered in ground-based observation dating back to 1998 while confirming the TESS detection of GJ 357 b, a “hot planet” that orbits much closer to the parent star. Even though GJ 357 d is 20% closer to GJ 357 than Earth is to the Sun, GJ 357 is much smaller than the Sun, receiving only as much energy as Mars. As a result, it is estimated that the average temperature is -64°F (-53°C), but this temperature is survivable for humans; if there is a thick enough atmosphere, the actual temperature could be much higher. If humans traveled there using modern spacecraft, it would take them about 660,000 years to get there. The planet is 6.1 times more massive than Earth and 2.3 times Earth's size.

Footnotes

References

Illustrations

Worked examples

Example 1 — a first encounter with Gliese 357 d

Start with the simplest possible case. Write down what Gliese 357 d 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 Gliese 357 d 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 Gliese 357 d 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 Gliese 357 d

In research: Gliese 357 d 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 Gliese 357 d 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: Gliese 357 d is common in secondary-school and first-year university syllabi. It links to neighbouring topics Exoplanet stubs, Exoplanets detected by radial velocity, Exoplanets discovered by TESS, so understanding it makes those chapters shorter.
In everyday life: Look for Gliese 357 d 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 Gliese 357 d in 20 minutes

Read the reference excerpt below once, without taking notes.
Close the page and write down what Gliese 357 d 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 Gliese 357 d out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Gliese 357 d in simple terms?

Why does Gliese 357 d 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 Gliese 357 d?

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 Gliese 357 d.