HeliocodexBack out to the solar system

Second planet · 0.72 au from the Sun

Venus

Nearly the same size as Earth, and the hottest planet there is. Almost everything we know about the ground comes from machines that lasted a couple of hours.

Backwards, and slowly

Venus turns the opposite way to most planets, and so slowly that one turn takes 243 Earth days. Its year is only 225. From one sunrise to the next is about 117 days, and the Sun comes up in the west.

The clouds do not wait. They race around the whole planet in roughly four days, much faster than the ground beneath them turns.

A sky of acid

The cloud deck is sulphuric acid, a thick yellow-white layer between about 50 and 70 km up. Around 50 km, where you would first dip below it, the pressure is close to one Earth atmosphere and the temperature is about that of a warm room. It is the most Earth-like place anywhere else in the solar system, which is why people have drawn up plans for floating habitats there.

Go lower and the air clears, and keeps getting heavier.

Down there

At the surface it is 464 °C, day and night, everywhere. That is hot enough to melt lead. The pressure is 92 times Earth’s, the same as being about 900 metres under the sea.

The light is dim and orange, a bit like a heavy overcast day, because the thick clouds and air strip out most of the blue. The wind is slow, about a metre a second. But the air is so dense that even that pushes like a gentle river.

The ground and sky here are generated, modelled on the photographs the Venera landers sent back: flat plates of rock under a dim orange sky.

What the radar saw

Soviet landers sent back the only photographs from the surface, in the 1970s and early 1980s. The longest-lived, Venera 13, worked for 127 minutes. To see the rest we use radar, which goes through cloud. NASA’s Magellan spacecraft mapped almost the whole planet that way between 1990 and 1994.

It found a young surface of lava plains and thousands of volcanoes, with far fewer craters than the Moon or Mars. Much of the planet seems to have been resurfaced a few hundred million years ago.

A computer-generated view across orange lava plains toward the broad dome of the volcano Maat Mons under a black sky.
Maat Mons, one of the largest volcanoes on Venus. Computer-generated from Magellan radar data, with the height exaggerated and colour added. Image: NASA/JPL.

In numbers

Radius
6,052 km
Mass
4.867 × 10²⁴ kg
Gravity at the surface
8.87 m/s²
Distance from the Sun
0.7233 au
A year
225 days
One turn on its axis
243 days, backwards
Sunrise to sunrise
117 days
Surface temperature
464 °C
Surface pressure
92 bar
Moons
0

NASA NSSDC Venus Fact Sheet and JPL orbital elements. Magellan image from NASA/JPL.