
Venus
Earth's scorching twin with a runaway greenhouse effect, retrograde rotation, and surface temperatures hot enough to melt lead.
About
Orbital Data
Physical Properties
Atmosphere
Venus has an extremely dense atmosphere composed of 96.5% carbon dioxide and 3.5% nitrogen, with traces of sulfur dioxide. The atmospheric pressure at the surface is about 92 times that of Earth -- equivalent to being nearly 1 km underwater on Earth. Thick clouds of sulfuric acid completely blanket the planet, trapping heat through an extreme greenhouse effect that makes Venus the hottest planet in the solar system.
Fun Facts
Venus spins so slowly that its day (243 Earth days) is longer than its year (225 Earth days).
Venus is the hottest planet in the solar system at 462°C, despite Mercury being closer to the Sun.
Venus rotates in the opposite direction to most planets, so the Sun rises in the west and sets in the east.
The atmospheric pressure on Venus's surface is 92 times that of Earth -- like being 900 meters underwater.
Venus has over 1,600 major volcanoes, more than any other planet in the solar system.
A year on Venus is shorter than a single Venusian solar day.
Venus is the brightest planet visible from Earth and can even cast shadows on very dark nights.
Soviet Venera landers survived on Venus's surface for up to 127 minutes before succumbing to the extreme conditions.
Compare
How does Venus stack up?