Mercury Planet Profile

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Questions and Answers

How long does it take for Venus to rotate once?

  • 88 Earth days
  • 59 Earth days
  • 243 Earth days (correct)
  • 224.7 Earth days

What is the primary gas that makes up Venus's suffocating atmosphere?

  • Nitrogen
  • Oxygen
  • Hydrogen
  • Carbon dioxide (correct)

Compared to most other planets, how does Venus spin on its axis?

  • Clockwise (correct)
  • Rapidly
  • Stationary
  • Counterclockwise

What is the average distance of Venus from the Sun?

<p>58 million km (B)</p> Signup and view all the answers

What is the surface temperature range of Venus?

<p>-180°C to 430°C (B)</p> Signup and view all the answers

Which planet has similar characteristics to Earth but has a suffocating atmosphere with sulfuric acid clouds?

<p>Venus (A)</p> Signup and view all the answers

What is the most likely reason why Mercury is hard to see in the sky?

<p>Its small size makes it difficult to spot against the Sun's glare. (B)</p> Signup and view all the answers

Why is Mercury denser than most planets, except Earth?

<p>It has a large core of iron and nickel, covered by a rocky mantle and crust. (A)</p> Signup and view all the answers

What makes Mercury's magnetic field weaker compared to Earth's?

<p>The planet spins more slowly on its axis. (A)</p> Signup and view all the answers

How does Mercury's surface compare to the Moon's?

<p>It has more impact basins and craters like the Moon. (D)</p> Signup and view all the answers

Which of the following statements accurately describes Venus compared to Earth?

<p>Venus has a runaway greenhouse effect, making it much hotter than Earth. (C)</p> Signup and view all the answers

How many times could Mercury fit into Earth based on their respective sizes?

<p>Approximately 18 times (B)</p> Signup and view all the answers

What is the reason why Venus doesn't appear to have many impact craters?

<p>Meteorites burn up in the thick atmosphere before reaching the surface. (C)</p> Signup and view all the answers

Which feature is NOT mentioned as observable on the surface of Venus?

<p>Mountains (B)</p> Signup and view all the answers

What distinguishes Aphrodite Terra on Venus?

<p>It is the largest highland region on Venus. (D)</p> Signup and view all the answers

Why have all the earlier probes sent to Venus been destroyed?

<p>Destroyed by extreme heat and pressure (B)</p> Signup and view all the answers

Which of the following is true about Venus's volcanoes?

<p>There are over 1,600 volcanoes on Venus. (B)</p> Signup and view all the answers

Why might Venus have fewer impact craters compared to other planets?

<p>The surface is too young for many collisions with large meteorites. (C)</p> Signup and view all the answers

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Study Notes

Mercury

  • Mercury is the smallest planet in our solar system.
  • It is the closest planet to the Sun, making it difficult to see except at sunrise or sunset.
  • Mercury has no moons and is too small to maintain an atmosphere.
  • It is denser than any planet except Earth, with a large iron and nickel core covered by a rocky mantle and crust.
  • Mercury's iron core produces a magnetic field that is 100 times weaker than Earth's.
  • The planet is covered with craters, including the giant Caloris Basin, which is about 800 miles (1,300 km) across.
  • The Caloris Basin's floor shows ridges and fractures, with mountains around the edge.

Venus

  • As our closest neighbor, Venus is an obvious place to send space probes.
  • The first successful landing on Venus was in 1970, and orbiters have used radar to peer through the thick cloud and reveal the surface since 1978.
  • Venus has at least 1,600 volcanoes, with the tallest being Maat Mons, about 3 miles (5 km) high.
  • The planet's highlands and lowlands include Aphrodite Terra, a highland region that runs two-thirds of the way around Venus.
  • Venus has few impact craters, possibly due to meteorites burning up in the thick atmosphere or the surface being too young to have had many collisions.
  • Most of the craters on Venus are less than 500 million years old.

Planet Profile: Venus

  • Average distance from the Sun: 58 million km
  • Surface temperature: -180°C to 430°C
  • Diameter: 4,875 km
  • Length of day: 59 Earth days
  • Length of year: 88 Earth days
  • Number of moons: 0
  • Gravity at the surface (Earth = 1): 0.38
  • Size comparison: Venus is similar in size, mass, and composition to Earth, but has no water or life and is covered with a thick atmosphere.

Key Features of Venus

  • Venus has a thick, suffocating atmosphere composed of sulfuric acid and carbon dioxide gas.
  • The atmosphere traps the Sun's heat, making it extremely hot.
  • The surface of Venus is hidden by a dense layer of pale yellow clouds made of sulfur and sulfuric acid.
  • Winds move the clouds around the planet from east to west at about 220 mph (350 km/h).
  • Venus spins very slowly clockwise, taking 243 Earth days to rotate once, making its day longer than its year.

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