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Schiaparelli (Martian crater)

Schiaparelli (Martian crater) is a science 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 Schiaparelli (Martian crater) rather than just read about it. In short: Schiaparelli ( SKAP-ə-REL-ee, SHAP-, US also skee-AHP-, Italian: [skjapaˈrɛlli]) is an impact crater on Mars, located near the planet's equator at latitude 2.7° south and longitude 16.7° east in the Sinus Sabaeus quadrangle. It measures approximately 459 kilometers (285-miles) in diameter and was named after Italian astronomer Giovanni Schiaparelli, known for his observations of the Red Planet and his mistranslated…

Schiaparelli (Martian crater) — main illustration
Schiaparelli (Martian crater) — illustration

Key takeaways

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

Reference excerpt

Schiaparelli ( SKAP-ə-REL-ee, SHAP-, US also skee-AHP-, Italian: [skjapaˈrɛlli]) is an impact crater on Mars, located near the planet's equator at latitude 2.7° south and longitude 16.7° east in the Sinus Sabaeus quadrangle. It measures approximately 459 kilometers (285-miles) in diameter and was named after Italian astronomer Giovanni Schiaparelli, known for his observations of the Red Planet and his mistranslated term "canali". The name was adopted by IAU's Working Group for Planetary System Nomenclature in 1973.

Description A crater within Schiaparelli shows many layers that may have formed by the wind, volcanoes, or deposition under water. Layers can be a few meters thick or tens of meters thick. Recent research on these layers suggests that ancient climate change on Mars, caused by regular variation in the planet's tilt, may have caused the patterns in layers. On Earth, similar changes (astronomical forcing) of climate results in ice-age cycles and formation of rhythmites. The regular appearance of rock layers suggests that regular changes in climate may be the root cause. Regular changes in climate may be due to variations of a planet's tilt (called obliquity). The tilt of the Earth's axis changes by only a little more than 2 degrees since the Moon is relatively large. In contrast Mars's tilt varies by tens of degrees. When the tilt is low (current situation on Mars), the poles are the coldest places on the planet, while the equator is the warmest (as on Earth). This could cause gases in the atmosphere, like water and carbon dioxide, to migrate poleward, where they would freeze. When the obliquity is higher, the poles receive more sunlight, causing those materials to migrate away. When carbon dioxide moves from the Martian poles, the atmospheric pressure increases, possibly causing a difference in the ability of winds to transport and deposit sand. Also, with more water in the atmosphere sand grains may stick and cement together to form layers.

Location on Mars

In popular culture In the 2011 novel The Martian by Andy Weir, and the 2015 feature film adapted from it, Schiaparelli is the landing site for Ares 4, the fourth crewed mission to Mars. The protagonist, Mark Watney, an astronaut from Ares 3 who is stranded on Mars, must travel from Acidalia Planitia to Schiaparelli, a journey of 3,200 kilometres (2,000 mi).

See also 4062 Schiaparelli, asteroid Climate of Mars Geology of Mars HiRISE HiWish program Impact event List of craters on Mars Ore resources on Mars Planetary nomenclature

References

External links Layers, Bedrock Ridges, and Dark Sand in Schiaparelli Crater, LPL HiRISE, includes large color photos

Illustrations

Schiaparelli (Martian crater) illustration
Schiaparelli (Martian crater): The Martian crater Schiaparelli is in the center of this 1980 mosaic from the Viking orbiter.
The Martian crater Schiaparelli is in the center of this 1980 mosaic from the Viking orbiter.
Schiaparelli (Martian crater) illustration

Worked examples

Example 1 — a first encounter with Schiaparelli (Martian crater)

Start with the simplest possible case. Write down what Schiaparelli (Martian crater) claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In science, 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 Schiaparelli (Martian crater) 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 Schiaparelli (Martian crater) 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 Schiaparelli (Martian crater)

In research
Schiaparelli (Martian crater) appears in science 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 Schiaparelli (Martian crater) 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
Schiaparelli (Martian crater) is common in secondary-school and first-year university syllabi. It links to neighbouring topics Impact craters on Mars, Sinus Sabaeus quadrangle, so understanding it makes those chapters shorter.
In everyday life
Look for Schiaparelli (Martian crater) 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 Schiaparelli (Martian crater) in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what Schiaparelli (Martian crater) 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 Schiaparelli (Martian crater) out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Schiaparelli (Martian crater) in simple terms?

Schiaparelli ( SKAP-ə-REL-ee, SHAP-, US also skee-AHP-, Italian: [skjapaˈrɛlli]) is an impact crater on Mars, located near the planet's equator at latitude 2.7° south and longitude 16.7° east in the Sinus Sabaeus quadrangle. It measures approximately 459 kilometers (285-miles) in diameter and was n…

Why does Schiaparelli (Martian crater) matter?

Because it connects several science 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 Schiaparelli (Martian crater)?

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 Schiaparelli (Martian crater).

Tags

  • Impact craters on Mars
  • Sinus Sabaeus quadrangle

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