✦ UNIVERSO FACILE
VENUS NOW

SOLAR SYSTEM / PLANET

VENUS

A world hidden beneath clouds

Venus is similar in size to Earth, yet its dense carbon-dioxide atmosphere produces an intense greenhouse effect. Clouds conceal its surface in visible light.

Generated illustration · not a photograph
← EXPLORE THE SOLAR SYSTEM
PROFILE · MEAN RADIUS6,052 km

NASA mean radius.

Getting to know Venus

A dense atmosphere, made mostly of carbon dioxide, traps heat through a strong greenhouse effect. Clouds hide the ground in visible light, but radar can reveal its topography.

Exploration and missions

The Magellan spacecraft used radar to map much of the surface and study volcanoes, plains and geological structures hidden beneath the clouds.

NASA Science · Venus ↗

FACTS TO EXPLORE

ORBITAL PERIOD0.615 Earth years
MEAN DISTANCE FROM THE SUN108.2 million km

Values are rounded. AU means astronomical unit. NASA source ↗

Credit: NASA / JPL-Caltech · NASA image record ↗

A greenhouse effect on a grand scale

Venus’s atmosphere is composed mostly of carbon dioxide, and its surface pressure is extremely high. Sunlight warms the planet; the atmosphere absorbs and re-emits some of the energy radiated by the surface, slowing heat loss. This powerful greenhouse effect helps make Venus hotter than Mercury, even though Venus is farther from the Sun. A planet’s distance from its star alone is not enough to predict its climate.

Looking beneath the clouds

Venus’s clouds hide the ground in visible light. To map it, Magellan sent radar pulses towards the surface and measured the returning signal: a way of “seeing” with radio waves rather than taking visible-light photographs. The topography reveals volcanoes, plains and deformed structures. Comparing different observations helps researchers investigate how and when the surface changed and whether some processes remain active.

Explore the official NASA source ↗