PLANETARY
FIELD NOTES
Cloud-covered Venus photographed by Mariner 10
The solar system / Planet 02

Venus

Earth's twin. A world apart.

Behind a brilliant veil of clouds lies the hottest planet in our solar system.

Explore the planet   ↓

Image: Venus, Mariner 10 · NASA/JPL-Caltech

12,104 kmEquatorial diameter
225 daysYear · Earth days
467 °CApprox. surface temperature
0 moonsNatural satellites
01 / A closer look

Familiar size.
Unfamiliar extremes.

01 /

A heat-trapping sky

A dense carbon dioxide atmosphere and sulfuric acid clouds surround this rocky world.

02 /

Crushing pressure

Surface air pressure is about 93 times Earth's sea-level pressure.

03 /

A backward spin

Venus rotates in the opposite direction to Earth. The Sun would rise in the west.

02 / The rhythm of a planet

One rotation
outlasts one year.

Venus takes about 243 Earth days to turn once, but only 225 to orbit the Sun.

One rotation243 Earth days
One orbit225 Earth days

Rotation period is measured relative to the stars.

03 / Exploration milestones

Getting to know
another world.

1962

Mariner 2

First successful flyby of another planet.

1970

Venera 7

First successful data transmission from another planet's surface.

1990

Magellan

Radar mapping begins to reveal the surface beneath the clouds.

Why does Venus look so bright?

Its clouds reflect sunlight strongly. Seen from Earth, Venus appears near sunrise or sunset.