Phobos
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| Phobos | |
|---|---|
| |
| Phobos by Viking Orbiter | |
| Date of discovery | August 18, 187718 August 1877 9 Elul 5637 H 9 Elul 6035 AM |
| Name of discoverer | Asaph Hall |
| Name origin | Greek phobos fear; attendant of Greek god of war |
| Orbital characteristics | |
| Celestial class | Moon |
| Primary | Mars |
| Order from primary | 1 |
| Periareion | 9236.39 km6.17415e-5 AU 5,739.227 mi[1] |
| Apoareion | 9519.61 km6.36347e-5 AU 5,915.211 mi[1] |
| Semi-major axis | 9,378 km6.26881e-5 AU 5,827.219 mi[2] |
| Orbital eccentricity | 0.0151 |
| Sidereal month | 0.3189 da8.73101e-4 a[2] |
| Synodic month | 0.3191 da8.73648e-4 a |
| Avg. orbital speed | 2.138 km/s7,696.8 km/h 1.328 mi/s 4,782.57 mph |
| Inclination | 1.093°0.0191 rad 1.214 grad to Mars's equator |
| Rotational characteristics | |
| Sidereal day | 0.3189 da7.654 h |
| Rotation speed | 11.0 km/h0.00306 km/s 0.0019 mi/s 6.835 mph |
| Axial tilt | 0°0 rad 0 grad |
| Physical characteristics | |
| Mass | 1.073 * 1016 kg1.4602e-7 M☾ 1.79552e-9 M⊕[1] |
| Mean density | 1,872 kg/m³1.872 g/ml 116.865 lb/ft³[3] |
| Mean radius | 11.1 km6.897 mi[3] |
| Surface gravity | 5.81e-3 m/s²0.0191 ft/s² 5.92455e-4 g[1] |
| Escape speed | 0.0114 km/s41.04 km/h 0.00708 mi/s 25.501 mph[1] |
| Surface area | 2997 km²1,157.148 mi² 7.90369e-5 A☾ 5.87564e-6 A⊕[1] |
| Minimum temperature | 161 K-112.15 °C -169.87 °F 289.8 °R[4] |
| Mean temperature | 233 K-40.15 °C -40.27 °F 419.4 °R |
| Maximum temperature | 269 K-4.15 °C 24.53 °F 484.2 °R[4] |
| Composition | Rock and ice mix |
| Color | #999999 |
| Albedo | 0.071[3] |
Phobos (from the Greek φόβος or phobos fear) is the inner, and the larger, of the two moons of Mars.
Contents |
Discovery
Phobos was discovered by the astronomer Asaph Hall on August 18, 1877, at the United States Naval Observatory in Washington, DC.[5][6][7] Astronomers were especially excited by the very short sidereal month of Phobos--about one-third of a Martian sidereal day--a phenomenon without precedent at the time.
The astronomer V. Knorre named the satellite Phobos (and also provided the name Deimos for the other satellite that Hall had discovered six days earlier), per a suggestion by Henry G. Madan of Eton, based on the names given in The Iliad for the two servants of Ares, the Greek god of war, named Fear (Phobos) and Panic (Deimos).[8]
Orbital and physical characteristics
Phobos orbits Mars at a distance closer than the distance of a synchronous orbit. For that reason, Phobos actually rises in the west and sets in the east of the Martian sky.[9] Yet because Phobos orbits Mars so closely, it is not visible above the horizon at latitudes higher than 70° north or south.
Phobos is not round, but is shaped like a potato, with dimensions 27 x 21.6 x 18.8 km. Its most remarkable surface feature is Crater Stickney, named for the family of Mrs. Asaph Hall. Stickney has a diameter of 10 km, and its outer rim has pronounced surface striations suggesting a tremendous impact.[10][9]
Phobos is spiraling in toward Mars at a rate of 18 mm per year. At that rate, if it had 50 million years to wait, it would enter the Martian atmosphere and drop to the surface in a cataclysmic crash, or else disintegrate into a ring.[4]
Origin
The favored theory among conventional astronomers is that Phobos and its companion moon Deimos are captured C-type asteroids.[4][9] However, that theory is not universally accepted.[4]
The Soviet spacecraft Phobos 2 discovered that Phobos was venting something into space, but all its systems failed before its controllers could determine what that substance was--most commentators believe that it was water.
In the 1950's and 1960's, a number of American and Soviet astrophysicists actually speculated that Phobos was hollow, and even that it was an artificial construct.[11] This speculation had part of its basis on a lack of understanding of Phobos' density and a gross overestimation of the rate of Phobos' orbital decay--5 cm per year instead of the 1.8 cm per year that present observations have established.
Exploration
The NASA Viking 1 orbiter took the first close-up photographs of Phobos on its way to deliver a landing craft to the Martian surface. Since then, several missions have made flybys of Phobos, including the orbiter that services the Spirit and Opportunity rovers, and the European Space Agency's Mars Express.[12][13]
Gallery
 Successive views of Phobos photographed from the surface of Mars by the Spirit Mars rover |
 High-resolution of Phobos from the camera in the Mars Orbiter now in orbit around Mars |
References
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| The Solar System | ||
| Star | Sol | |
| Factitious Planet | Vulcan | |
| Terrestrial Planets | Mercury • Venus • Earth • Mars | |
| Gas giants | Jupiter • Saturn • Uranus • Neptune | |
| Dwarf Planets | Ceres • Pluto • Eris | |
| Asteroid Belt | Major asteroids • C-type asteroids • S-type asteroids • M-type asteroids | |
| Trans-Neptunian Objects | Kuiper belt • Scattered disk • Oort cloud • Nemesis | |
| Moons | Terrestrial • Martian • Jovian • Saturnine • Uranian • Neptunian • Plutonian • Eridian | |
| Featured moons | Moon • Phobos • Deimos • Io • Europa • Ganymede • Callisto • Mimas • Enceladus • Tethys • Dione • Rhea • Titan • Hyperion • Iapetus • Miranda • Ariel • Umbriel • Titania • Oberon • Triton • Nereid • Charon • Nix • Hydra • Dysnomia |
| The Martian System | ||
| Primary | Mars | |
| Moons | Phobos • Deimos |
Categories: Astronomy | Solar system | Moon | Mars
