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Surface

Surface

Froms space, Venus is bright white because it is covered with clouds that reflect and scatter sunlight. At the surface, the rocks are different shades of grey, like rocks on Earth, but the thick atmosphere filters the sunlight so that everything would look orange if you were standing on Venus.

Venus has mountains, valleys, and tens of thousands of volcanoes. The highest mountain on Venus, Maxwell Montes, is 20,000 feet high (8.8 kilometers), similar to the highest mountain on Earth, Mount Everest. The landscape is dusty, and surface temperatures reach a scalding 880 degrees Fahrenheit (470 degrees Celsius).

Venus is covered in craters, but none are smaller than 0.9 to 1.2 miles (1.5 to 2 kilometers) across. Small meteoroids burn up in the dense atmosphere, so only large meteoroids reach the surface and create impact craters.

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Venus

Venus

Venus is the second planet from the Sun and our closest planetary neighbor. 

Similar in structure and size to Earth, Venus spins slowly in the opposite direction from most planets. 

Its thick atmosphere traps heat in a runaway greenhouse effect, making it the hottest planet in our sol...

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Size and distance

Size and distance

With a radius of 3,760 miles (6,052 kilometers), Venus is roughly the same size as Earth — just slightly smaller.

From an average distance of 67 million miles (108 million kilometers), Venus is 0.7 astronomical units away from the Sun. One astronomical unit (abbreviated as AU), is the dista...

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Quick facts

Day: 243 Earth days

Year: 225 Earth days

Radius: 3,760 miles | 6,052 kilometers

Planet type: Terrestrial

Temperature: 880 degrees Fahrenheit / 471 degrees Celsius

Moons:

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Formation

Formation

When the solar system settled into its current layout about 4.5 billion years ago, Venus formed when gravity pulled swirling gas and dust together to form the second planet from the Sun. 

Like its fellow terrestrial planets, Venus has a central core, a rocky mantle and a solid crust.

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Orbit and rotation

Orbit and rotation

Venus rotation and orbit are unusual in several ways, Venus is one of just two planets that rotate from east to west.

 Only Venus and Uranus have this "backwards" rotation. It completes one rotation in 243 Earth days — the longest day of any planet in our solar system, even longer than a wh...

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Atmosphere

Atmosphere

Venus atmosphere consists mainly of carbon dioxide, with clouds of sulfuric acid droplets

The thick atmosphere traps the Sun's heat, resulting in surface temperatures higher than 880 degrees Fahrenheit (470 degrees Celsius). The atmosphere has many layers with different temperatures. At the...

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Moons

Venus has no moons.

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Magnetosphere

Even tho venus is similar in size to the Earth and has a similarly-sized iron core, Venus' magnetic field is much weaker than the Earth's due to Venus' slow rotation. ​

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Structure

Venus is in many ways similar to earth in its structure. 

It has an iron core that is approximately 2,000 miles (3,200 kilometers) in radius. Above that is a mantle made of hot rock slowly churning due to the planet's interior heat. 

The surface is a thin crust of rock that bulges and...

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Rings

Venus has no rings.

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Potential for life

Potential for life

No human has ever visited venus, but the spacecrafts taht have been sent to the surface of Venus do not last very long there. Venus' high surface temperatures overheat electronics in spacecraft in a short time, so it seems unlikely that a person could survive for long on the Venusian surface.

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CURATED FROM

Venus

Venus

solarsystem.nasa.gov

12 ideas

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IDEAS CURATED BY

rogierhoekstra

I'm passionate about helping people live their best lives. I'm a lifestyle coach and fitness trainer, and I also write and take photographs. Check out the link below for more and follow me on twitter!

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Surface

Surface

The red planet is actually many colors. At the surface, we see colors as brown, gold, and tan. The reason Mars looks reddish is due to oxidization—or rusting—of iron in the rocks, regolith (Martian “soil”), and dust of Mars. This dust gets kicked up into the atmosphere and from a distance makes t...

5 Need-to-Know Facts about MERCURY.

On mercury Daytime Temperatures can reach 430 degrees Celsius and drop to -180 degrees Celsius at night.

One day-night cycle on Mercury takes 175.97 Earth days and a year of Mercury is just 88 Earth days. 

Standing on Mercury's surface at its closest approach to the Sun, our star woul...

The Sun’s atmosphere is hotter than its surface

The Sun’s atmosphere is hotter than its surface

The visible surface of the Sun (the photosphere) is around 6,000°C. But a few thousand kilometers above it – a small distance when we consider the size of the Sun – the solar atmosphere (the corona) is hundreds of times hotter, reaching a...

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