Venus
Welcome to Venus, 11 meters from the Sun, and 1.2 mm wide.
The Planetfield is a unique light model of our solar system, at the correct relative scale, where both distances and planet sizes are reduced by a factor of ten billion. Read more about the model.
Venus is the planet that gets closest to Earth, and it is the brightest object in the sky after the Sun and the Moon. It is a rocky planet covered by a thick, yellowish-white cloud layer that makes it impossible to see the surface in visible light. The planet’s dense atmosphere consists mostly of carbon dioxide, about 3.5 per cent nitrogen, and a small amount of sulfur dioxide (in the form of a corrosive sulfuric acid mist). This atmosphere acts as an extreme greenhouse, preventing heat from escaping. Venus is therefore the hottest planet in the Solar System, with a stable surface temperature of around 465 °C. That is hot enough to melt lead and make the ground glow in the dark. In addition, atmospheric pressure at the surface is as much as 93 times greater than at sea level on Earth.
Nevertheless, we know a great deal about the surface. In the early 1990s, the Magellan space probe mapped the planet using radar and revealed a dramatic landscape of plains, mountains, meteorite craters, and more than a thousand volcanic structures. In recent years, scientists have found concrete evidence that some of these volcanoes are still active today.
Although conditions on the surface are extremely inhospitable, conditions are very different 50 kilometers up in the atmosphere. Winds there rage at speeds of up to 360 km/h, but the temperature (30–70 °C) and air pressure resemble those at Earth’s surface. Scientists have even speculated that mysterious dark streaks in the clouds, which absorb ultraviolet radiation, could theoretically be caused by acid-tolerant microbes or bacteria.
Venus has an average distance from the Sun of 108 million kilometers. Spending a day there would be confusing: the planet rotates extremely slowly and in the opposite direction to most other planets, meaning that the Sun rises in the west and sets in the east. One full day lasts 243 Earth days, which is actually longer than a Venusian year of 225 Earth days. Why the planet rotates “the wrong way” remains a mystery. One explanation could be that the planet collided with another large object early in the history of the solar system.
Since its axial tilt is only three degrees, Venus also has no noticeable seasons. Along with Mercury, Venus is also one of the only planets in the Solar System with no moons of its own.
Facts about Venus
| Diameter | 12 104 km |
|---|---|
| Distance from the Sun | About 108 millions of kms |
| Rotation period | 243 Earth days |
| Orbital period around the Sun | 225 Earth days |
| Surface temperature | About 465 ºC |