Mars
Mars is the fourth planet from the Sun, a rocky world with a thin, carbon-dioxide-rich atmosphere and a surface colored red by oxidized iron minerals. Its day is close in length to Earth's, but its year is longer, and it has two small moons, Phobos and Deimos. Geological features and minerals record a past in which liquid water was more widespread. A 2025 peer-reviewed study reported potential biosignatures in a Perseverance sample, but these are not proof of life and require further study.
A terrestrial planet
Mars is the fourth planet outward from the Sun and one of the Solar System's rocky, or terrestrial, planets. Its radius is about half Earth's. A Martian rotation takes about 24.6 hours, while one orbit around the Sun takes about 687 Earth days. Its tilted axis gives it seasons, though they last longer than Earth's because the Martian year is longer. The planet has two small, irregularly shaped moons, Phobos and Deimos. Iron-bearing minerals in Martian rocks and dust oxidize, giving much of the surface its familiar reddish appearance.
Surface, atmosphere and water
Mars has a thin atmosphere composed mostly of carbon dioxide, with nitrogen and argon among its other gases. Its landscape includes impact craters, enormous volcanoes such as Olympus Mons and the canyon system Valles Marineris. Landforms such as ancient river valleys, deltas and lakebeds, together with minerals formed in water, are evidence that liquid water once flowed or collected on the surface. Water is present today chiefly as ice, including at the poles and beneath the surface; the low atmospheric pressure makes persistent liquid water on the open surface difficult. Dust and weather continue to modify the landscape.
A record of planetary change
Mars preserves evidence useful for studying how rocky planets evolve. Its surface records impacts, volcanic activity and ancient water-related processes, while its thin atmosphere and present cold, dry conditions contrast with evidence for a warmer, wetter past. Orbital observations, surface geology and atmospheric measurements address how that transition occurred and what conditions might once have been habitable. The question of life remains open. A 2025 peer-reviewed study of the Perseverance rover's “Sapphire Canyon” core, collected from the Cheyava Falls rock in Jezero Crater, described mineral and organic associations as potential biosignatures. NASA and the researchers stressed that a potential biosignature is not proof of life; further study, including analysis with laboratory instruments on Earth, is needed to determine the materials' origin. Earlier, NASA's Viking landers found no clear evidence of living microorganisms in soil near their landing sites.
Exploration
Knowledge of Mars has grown from telescopic observation to robotic missions using flybys, orbiters, landers and rovers. NASA's Mariner 4 returned the first spacecraft images of Mars during a flyby in 1965. In 1976, Viking 1 became the first U.S. mission to land safely on the planet and send images from its surface. Later international orbiters and rovers have mapped terrain, analyzed rocks and soils, and measured the atmosphere. ESA's Mars Express, in orbit since 2003 and conducting science operations from 2004, has mapped atmospheric chemistry and investigated the planet's history of water. These missions help scientists assess Mars as a world in its own right and plan future exploration.
Key facts
- Position
- Mars is the fourth planet from the Sun.
- Day and year
- A rotation takes about 24.6 hours; an orbit takes about 687 Earth days.
- Moons
- Mars has two small moons: Phobos and Deimos.
- Atmosphere
- The thin atmosphere is composed mostly of carbon dioxide.
- Water evidence
- Surface features and minerals record a wetter past; present-day water is found chiefly as ice.
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References
- 1.Mars: Facts
NASA Science · other · reliability: high · retrieved 14 October 2026
Supports: Planetary basics, rotation and orbit, moons, atmosphere, surface features and evidence for water on Mars.
- 2.Mars Facts, Surface, Moons, Temperature, & Atmosphere
Encyclopaedia Britannica · other · reliability: high · retrieved 14 October 2026
Supports: Reference overview of the planet's astronomical characteristics, surface, atmosphere and geological features.
- 3.Mars Exploration Program
NASA Science · other · reliability: high · retrieved 14 October 2026
Supports: Mars exploration goals and a chronology of NASA missions, including Mariner 4 and later robotic missions.
- 4.Viking Project
NASA Science · other · reliability: high · retrieved 14 October 2026
Supports: Viking 1's landing and scientific work, including results of its experiments seeking evidence of life.
- 5.Mars Express
European Space Agency · other · reliability: high · retrieved 14 October 2026
Supports: Mars Express mission chronology and its observations of Mars's atmosphere, surface, moon Phobos and water history.
- 6.Redox-driven mineral and organic associations in Jezero Crater, Mars
Nature · other · reliability: high · retrieved 14 October 2026
Supports: Peer-reviewed analysis of mineral and organic associations in the Perseverance-collected Sapphire Canyon sample and the further analysis needed to determine their origin.
- 7.NASA Says Mars Rover Discovered Potential Biosignature Last Year
NASA · other · reliability: high · retrieved 14 October 2026
Supports: NASA describes the sample and clarifies that a potential biosignature requires further study before drawing conclusions about whether life is present or was present.
References are suggested by the research engine and may be incomplete. Unverified URLs are omitted rather than guessed.
Article history
- Version 114 October 2026 · EditorCreated by Zapia