Mars

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For the Roman god of war, see Mars (god)

Mars

Mars photographed by Viking Orbiters
Symbol
Name of discoverer Known to ancients
Name origin Roman god of war
Orbital characteristics
Primary Sun
Order from primary 4
Perihelion 206,644,545 km (1.381 AU)
Aphelion 249,228,730 km (1.666 AU)
Semi-major axis 227,936,637 km (1.524 AU)
Titius-Bode prediction 1.6 AU
Circumference 1,429,033,627 km
Orbital eccentricity 0.093
Sidereal year 686.96 da (1.881 a)
Synodic year 779.96 da (2.135 a)
Avg. orbital speed 24.077 km/s
Inclination 1.851° to the ecliptic
Rotational characteristics
Sidereal day 24.62296194 h (1.026 da)
Solar day 24.65979 h (1.027 da)
Rotational speed 465.11 m/s
Axial tilt 25.19°
Physical characteristics
Mass 6.4185 * 1023 kg (10.74% earth)
Density 3,943 kg/m³
Equatorial radius 3402.5 km
Surface gravity 3.72 m/s² (0.379 g)
Escape speed 5.02 km/s
Surface area 144,800,000 km² (28.388% earth)
Minimum temperature 186 K
Mean temperature 227 K
Maximum temperature 268 K
Number of moons 2
Composition Rock
Color Red
Albedo 0.15

Mars is the fourth planet from the Sun, after Mercury, Venus, and Earth. It is called "The Red Planet" because it looks red from Earth.

The planet has been known since Antiquity. Because of this, the planet was named after the Roman equivalent of Ares, the Greek god of war.

[edit] Physical and surface features

There is a dichotomy on the surface of Mars; the northern hemisphere consists of low-lying volcanic plains, with the southern hemisphere consists of ancient, heavily-cratered highland plains. Mars also has two volcanic regions: Tharsis and Elysium. Within the Tharsis region is the largest volcano in the solar system, Olympus Mons. Olympus Mons is approximately 500 km across and is about the same size as the state of Arizona. Its peak is 24 km above the surrounding plains and it is surrounded by a vertical scarp 6 km high. A large canyon system, Valles Marineris, is located along the Martian equator east of the Tharsis region. Valles Marineris is 2-6km deep and 200-600km wide and approximately 4,500 km long (approximately the distance from San Francisco to Boston). The eastern part of Valles Marineris appears to have a tectonic origin, but the western part is characterized by features such as teardrop islands and longitudinal grooves, indicating it may have been formed by catastrophic flooding in the past. Such flooding may be possible under current climate conditions. Run-off channels in the cratered highland indicate a thicker atmosphere or warmer climate in the past that would have allowed water to be stable on the surface.

Recent satellite imagery has shown that Mars has a 3 kilometer deep ice cap around its polar regions. The northern polar region is surrounded by dune fields. During the Martian winter, a layer of carbon dioxide condenses at the poles and sublimates in the summer, leaving the water-ice and dust polar caps exposed. The ratio of dust to water-ice contained in the polar caps remains unknown.

[edit] Satellites

Mars has two moons: Phobos and Deimos (which respectively mean "Fear and "Panic" in Greek). Russian scientists in the 1950s posited that Phobos might be hollow, but these claims were discredited in the late 1960s.

Topographic map of Mars.
Topographic map of Mars.
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