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Venus is the second closest planet to the Sun and has a similar size to Earth. It is named after the Roman goddess of love and beauty. It has a dense atmosphere of mainly carbon dioxide which retains a lot of the Sun’s heat, making it the hottest planet.

Venus is the second planet from the Sun. It is similar in size to the Earth and it also has a similar composition. Like our planet, Venus has a hot iron core surrounded by a mantle. The planet also has a dense atmosphere of mainly carbon dioxide which can retain a lot of the Sun’s heat making it the hottest planet in our solar system, with an average temperature of 464°C (867°F). It has the least elliptical orbit out of all the planets. After our own Moon, it is the brightest object in the night sky, which is perhaps why the planet is named after the Roman goddess of love and beauty.

Venus is the closest planet to Earth, with an average distance of 41 million km, but missions to Venus can be difficult due to the extreme temperatures found on the planet’s surface. There have been several unmanned missions to Venus. In 1970 the Soviet Union landed Venera 7, making it the first spacecraft to land on another planet. Between 1990-1994, the Magellan mission orbited the planet and managed to image 98% of the planet's surface.

A Venusian year lasts 224.7 Earth days. Venus and Uranus are interesting as the planets’ rotations on their axis are opposite to all other planets in the solar system. Venus has the longest day out of all other planets at 243 Earth days.

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Venus Facts

  • Orbital Period: 225 Earth days
  • Length of a Day:243 Earth days
  • Diameter: 12,104 km
  • Distance from the Sun: 108,000,000 km
  • Strength of Gravity: 8.9 N/kg
  • Number of Moons: 0

How Tos about Guide to Planet Venus

1

Engage students with a Venus model activity

Gather simple materials like clay, colored paper, and markers to represent Venus’s features. Explain the planet’s thick atmosphere and bright surface as students build their models for a hands-on learning experience.

2

Connect Venus facts to real-world science

Discuss Venus’s extreme temperatures and volcanic activity to spark conversations about climate and geology on Earth. Relate classroom lessons to current events like space missions for added relevance.

3

Use multimedia to visualize Venus

Show NASA videos or online images of Venus to help students see its clouds and surface. Encourage students to compare Venus’s appearance with other planets to deepen understanding.

4

Facilitate a Venus-themed group discussion

Pose questions about Venus’s rotation, atmosphere, and visibility in the night sky. Invite students to share their ideas and observations for active participation.

5

Assign a creative Venus research project

Ask students to create posters or short reports highlighting key facts about Venus. Encourage creativity and teamwork to reinforce what they’ve learned in a fun way.

Frequently Asked Questions about Guide to Planet Venus

What is Planet Venus?

Planet Venus is the second planet from the Sun and is known for its bright appearance and thick, toxic atmosphere. It's often called Earth's sister planet due to its similar size and structure.

Why is Venus called Earth's sister planet?

Venus is called Earth's sister planet because it is similar in size, mass, and composition to Earth, though its atmosphere and surface conditions are very different.

What makes Venus different from other planets in our solar system?

Venus stands out due to its thick carbon dioxide atmosphere, extremely high surface temperatures, and its rotation direction, which is opposite to most other planets.

How hot does it get on Venus?

Venus is the hottest planet in our solar system, with surface temperatures reaching up to 465°C (869°F) due to its dense greenhouse gas atmosphere.

Can humans land or survive on Venus?

Humans cannot land or survive on Venus because of its extreme heat, high atmospheric pressure, and acidic clouds, which make it an inhospitable environment for life as we know it.

Learn more about the stars and other celestial bodies in our Picture Encyclopedia of Astronomy Terms!
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