Venus
Terrestrial Planet

Venus

Earth's scorching twin with a runaway greenhouse effect, retrograde rotation, and surface temperatures hot enough to melt lead.

12,104km
Diameter
8.9m/s²
Surface Gravity
462°C
Mean Temperature
0
Known Moons

About

Venus is the second planet from the Sun and Earth's closest planetary neighbor. Often called Earth's 'sister planet' due to their similar size and mass, Venus is actually a radically different world. Its thick carbon dioxide atmosphere creates a runaway greenhouse effect that makes it the hottest planet in the solar system, with a near-uniform surface temperature of about 462°C -- hot enough to melt lead. The atmospheric pressure at the surface is a crushing 92 times that of Earth. Venus rotates backward compared to most planets (retrograde rotation), and it does so extremely slowly -- one Venusian day lasts 243 Earth days, which is actually longer than its year of 225 Earth days. This means the Sun rises in the west and sets in the east on Venus. The planet's surface, hidden beneath perpetual clouds of sulfuric acid, was mapped by radar from the Magellan spacecraft in the early 1990s, revealing a landscape of vast volcanic plains, highland regions, and thousands of volcanoes, some of which may still be active. Venus is the brightest natural object in Earth's night sky after the Moon, earning it the names 'Morning Star' and 'Evening Star' since ancient times. Despite its hellish conditions, some scientists have proposed that microbial life could potentially exist in the more temperate upper cloud layers, where temperatures and pressures are more Earth-like. In 2020, a controversial detection of phosphine gas in Venus's atmosphere sparked renewed interest in this possibility.

Orbital Data

0.723AU
Distance from Sun
224.7days
Orbital Period
35.0km/s
Orbital Velocity
0.0068
Eccentricity
2802.0hours
Day Length
177.4°
Axial Tilt
107.5 million km
Perihelion
108.9 million km
Aphelion

Physical Properties

0.815x
Mass (Earth = 1)
5.24g/cm³
Density
10.4km/s
Escape Velocity
0.9x
Volume (Earth = 1)
462°C
Min Temperature
462°C
Max Temperature
No
Ring System
-5832.5hours
Rotation Period

Atmosphere

Carbon Dioxide (96.5%)Nitrogen (3.5%)Sulfur DioxideArgonWater Vapor

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

01

Venus spins so slowly that its day (243 Earth days) is longer than its year (225 Earth days).

02

Venus is the hottest planet in the solar system at 462°C, despite Mercury being closer to the Sun.

03

Venus rotates in the opposite direction to most planets, so the Sun rises in the west and sets in the east.

04

The atmospheric pressure on Venus's surface is 92 times that of Earth -- like being 900 meters underwater.

05

Venus has over 1,600 major volcanoes, more than any other planet in the solar system.

06

A year on Venus is shorter than a single Venusian solar day.

07

Venus is the brightest planet visible from Earth and can even cast shadows on very dark nights.

08

Soviet Venera landers survived on Venus's surface for up to 127 minutes before succumbing to the extreme conditions.

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