CosmosObservatory
Explore
Solar System
Live
Learn
Tools
About
Cosmos Observatory
ToolsAbout
Cosmos Observatory

Explore the universe through NASA data, real-time ISS tracking, Mars rover imagery, asteroid monitoring, and comprehensive space encyclopedia. Your gateway to the cosmos.

Explore

  • APOD
  • Mars Rovers
  • Earth Imagery
  • NASA Gallery
  • ISS Tracker

Data

  • Asteroids
  • Solar System
  • Exoplanets
  • Space Weather
  • Launches

Tools

  • Glossary
  • News
  • Calculators

Legal

  • About
  • Privacy Policy
  • Terms of Use
  • Space Tools
  • Contact

Stay updated with the cosmos

Get weekly digests of APOD highlights, upcoming launches, and space events.

© 2026 Cosmos Observatory. All rights reserved. Built with for space enthusiasts.

This website is not affiliated with, maintained, authorized, endorsed by, or in any way officially connected with NASA or any of its subsidiaries or affiliates. All NASA imagery is in the public domain unless otherwise noted. Data sourced from NASA Open APIs, Launch Library 2, and other open data services.

  1. Home
  2. Solar System
  3. Venus
Terrestrial#2 from Sun

Venus ♀

Venus is the hottest planet in our solar system, with a thick toxic atmosphere that traps heat in a runaway greenhouse effect.

About Venus

Atmosphere

Venus has the densest atmosphere of any terrestrial planet, composed of roughly 96.5 percent carbon dioxide with clouds of sulfuric acid. The surface atmospheric pressure is about 92 times that of Earth, equivalent to being almost a kilometer beneath the ocean. A runaway greenhouse effect traps solar energy, heating the surface to an average of 464 degrees Celsius -- hot enough to melt lead and making Venus the hottest planet despite being farther from the Sun than Mercury.

Notable Features

Venus's surface is dominated by volcanic plains, with over 1,600 major volcanoes identified. Maxwell Montes, the highest mountain, rises about 11 km above the mean surface level. The planet rotates extremely slowly and in the opposite direction to most planets, so the Sun rises in the west and sets in the east. A single day on Venus (243 Earth days) is actually longer than a Venusian year (225 Earth days).

Exploration History

The Soviet Venera program achieved remarkable firsts at Venus, including the first atmospheric entry (Venera 4, 1967), first soft landing (Venera 7, 1970), and first surface photographs (Venera 9, 1975). NASA's Magellan mission (1990-1994) used radar to map 98 percent of the surface at high resolution. JAXA's Akatsuki orbiter continues to study the atmospheric dynamics. Future missions including NASA's VERITAS and ESA's EnVision aim to unlock remaining mysteries about Venus's geology and possible past habitability.

Physical Properties

Diameter

12,104 km

Mass (Earth = 1)

0.815

Surface Gravity

8.87 m/s²

Distance from Sun

0.72 AU

Orbital Period

225 days

Rotation Period

5,832 hours

Avg Temperature

464°C

Escape Velocity

10.36 km/s

Atmosphere Composition

Carbon DioxideNitrogenSulfuric Acid

How Does Venus Compare to Earth?

Diameter

Venus12,104 km
Earth12,756 km

1.05x smaller than Earth

Mass

Venus0.815x Earth
Earth1.000x

1.23x smaller than Earth

Surface Gravity

Venus8.87 m/s²
Earth9.81 m/s²

1.11x smaller than Earth

Did You Know?

01

Venus spins so slowly that a single day on Venus is longer than a Venusian year.

02

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

03

Venus is sometimes called Earth's "twin" because of their similar size and mass.

Missions to Venus

MissionYearAgencyStatus
Venera 71970USSRComplete
Magellan1990-1994NASAComplete
Akatsuki2015-presentJAXAActive
VERITASTBDNASAPlanned

Venus FAQ

Why does Venus spin backward?+
Venus has retrograde rotation, spinning clockwise when viewed from above its north pole, opposite to most planets. Scientists believe a massive collision early in Venus's history may have flipped its rotation, or tidal effects from its thick atmosphere and the Sun gradually reversed it over billions of years.
Could there be life on Venus?+
In 2020, scientists reported detecting phosphine gas in Venus's atmosphere, which on Earth is produced by living organisms. While the finding remains controversial, Venus's cloud layer at 50-60 km altitude has temperatures and pressures similar to Earth's surface, making it a potential habitat for extremophile microorganisms.
Why is Venus so hot?+
Venus's thick atmosphere of carbon dioxide creates an extreme greenhouse effect, trapping heat and raising surface temperatures to about 464 degrees Celsius. The atmospheric pressure is 92 times Earth's, and dense sulfuric acid clouds prevent heat from escaping back into space.

Fun Fact

“Venus rotates backwards compared to most planets, so the Sun rises in the west and sets in the east.”

MercuryEarth

All Planets

Exoplanets

ISS Tracker

Glossary