True-color view of Mars seen through NASA'sHubble Space Telescope in 1999.
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| Designations | |||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Pronunciation | |||||||||||||
| Adjective | Martian | ||||||||||||
| Orbital characteristics [2] | |||||||||||||
| Epoch J2000 | |||||||||||||
| Aphelion |
249,209,300 km (154,851,500 mi)
1.665 861 AU | ||||||||||||
| Perihelion |
206,669,000 km (128,418,000 mi)
1.381 497 AU | ||||||||||||
| Semi-major axis |
227,939,100 km (141,634,800 mi)
1.523 679 AU | ||||||||||||
| Eccentricity | 0.093 315 | ||||||||||||
| Orbital period |
686.971 days
668.5991 sols1.8808 Julian years | ||||||||||||
| Synodic period |
779.96 days
2.135 Julian years | ||||||||||||
| Average orbital speed | 24.077 km/s | ||||||||||||
| Mean anomaly | 19.3564° | ||||||||||||
| Inclination | 1.850° to ecliptic 5.65° to Sun's equator 1.67° to invariable plane[1] | ||||||||||||
| Longitude of ascending node | 49.562° | ||||||||||||
| Argument of perihelion | 286.537° | ||||||||||||
| Satellites | 2 | ||||||||||||
| Physical characteristics | |||||||||||||
| Equatorial radius | 0.533 Earths | ||||||||||||
| Polar radius | 0.531 Earths | ||||||||||||
| Flattening | 0.005 89 ± 0.000 15 | ||||||||||||
| Surface area |
144,798,500 km2
0.284 Earths | ||||||||||||
| Volume |
1.6318×1011 km3[4]
0.151 Earths | ||||||||||||
| Mass |
6.4185×1023 kg[4]
0.107 Earths | ||||||||||||
| Mean density | 3.9335 ± 0.0004[4] g/cm³ | ||||||||||||
| Equatorial surface gravity | 0.376 g | ||||||||||||
| Escape velocity | 5.027 km/s | ||||||||||||
| Sidereal rotation period |
1.025 957 day
24.622 9 h[4] | ||||||||||||
| Equatorial rotation velocity | 868.22 km/h (241.17 m/s) | ||||||||||||
| Axial tilt | 25.19° | ||||||||||||
| North poleright ascension |
21 h 10 min 44 s
317.681 43° | ||||||||||||
| North pole declination | 52.886 50° | ||||||||||||
| Albedo | 0.25 (Bond)[6] | ||||||||||||
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| Apparent magnitude | +1.6 to −3.0[7] | ||||||||||||
| Angular diameter | 3.5–25.1"[6] | ||||||||||||
| Atmosphere[6][13] | |||||||||||||
| Surface pressure | 0.636 (0.4–0.87) kPa | ||||||||||||
| Composition |
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Mars is the fourth planet from the Sun and the second smallest planet in the Solar System. Named after the Roman god of war, it is often described as the "Red Planet", as the iron oxide prevalent on its surface gives it a reddish appearance.[14] Mars is a terrestrial planet with a thinatmosphere, having surface features reminiscent both of the impact craters of the Moon and the volcanoes, valleys, deserts, and polar ice caps ofEarth. The rotational period and seasonal cycles of Mars are likewise similar to those of Earth, as is the tilt that produces the seasons. Mars is the site of Olympus Mons, the second highest known mountain within the Solar System (the tallest on a planet), and of Valles Marineris, one of the largest canyons. The smooth Borealis basin in the northern hemisphere covers 40% of the planet and may be a giant impact feature.[15][16] Mars has two known moons, Phobos and Deimos, which are small and irregularly shaped. These may be captured asteroids,[17][18] similar to 5261 Eureka, a Martian trojan asteroid.
Until the first successful Mars flyby in 1965 by Mariner 4, many speculated about the presence of liquid water on the planet's surface. This was based on observed periodic variations in light and dark patches, particularly in the polar latitudes, which appeared to be seas and continents; long, dark striations were interpreted by some as irrigation channels for liquid water. These straight line features were later explained as optical illusions, though geological evidence gathered by unmanned missions suggest that Mars once had large-scale water coverage on its surface.[19] In 2005, radar data revealed the presence of large quantities of water ice at the poles[20] and at mid-latitudes.[21][22] The Mars rover Spirit sampled chemical compounds containing water molecules in March 2007. The Phoenix lander directly sampled water ice in shallow Martian soil on July 31, 2008.[23]
Mars is currently host to five functioning spacecraft: three in orbit – the Mars Odyssey, Mars Express, and Mars Reconnaissance Orbiter; and two on the surface – Mars Exploration Rover Opportunity and the Mars Science Laboratory Curiosity. Defunct spacecraft on the surface include MER-ASpirit and several other inert landers and rovers such as the Phoenix lander, which completed its mission in 2008. Observations by the Mars Reconnaissance Orbiter have revealed possible flowing water during the warmest months on Mars.[24]
Mars can easily be seen from Earth with the naked eye, as can its reddish coloring. Its apparent magnitude reaches −3.0,[7] which is surpassed only by Jupiter, Venus, the Moon, and the Sun. Optical ground-based telescopes are typically limited to resolving features about 300 km (186 miles) across when Earth and Mars are closest because of Earth's atmosphere.[25]
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