| An image of Deimos taken by the Viking 1 orbiter. | |
| Discovery | |
|---|---|
| Discovered by | Asaph Hall |
| Discovered on | August 12 1877 |
| Orbital characteristics | |
| Mean radius | 23,460 km |
| Eccentricity | 0.0002 |
| Revolution period | 1.262 d |
| Avg. Orbital Speed | 0.22 km/s |
| Inclination | 0.93° (to Mars' equator) 1.793° (to the local Laplace plane) 27.58° (to the ecliptic) |
| Satellite of | Mars |
| Physical characteristics | |
| Mean diameter | 12.6 km (15.0×12×10.4) |
| Mass | 2.244 kg |
| Mean density | 2.2 g/cm3 |
| Surface gravity | 0.0039 m/s² (3.9 mm/s²) |
| Surface Gravity (Earth = 1) | 0.00040 (400 µg) |
| Escape velocity | 0.0069 km/s (6.9 m/s) |
| Rotation period | synchronous |
| Albedo | 0.07 |
| Surface temp. | ≈233 K |
| Atmospheric pressure | no atmosphere |
Deimos was discovered on August 12, 1877 at about 07:48 UTC (given in contemporary sources as "August 11 14:40" Washington mean time using the old astronomical convention of beginning a day at noon, so 12 hours must be added to get the actual local mean time) *.
Deimos is composed of carbon-rich rock, much like C-type (carbonaceous chondrite) asteroids, and ice. It is cratered, but the surface is noticeably smoother than that of Phobos, caused by the partial filling of craters with regolith. The two largest craters, Swift and Voltaire, measure about 3 kilometres across.
As seen from Deimos, Mars would be 1000 times larger and 400 times brighter than the full Moon as seen from Earth, taking up a full 1/11 of the width of a celestial hemisphere.
As seen from Mars, Deimos has an angular diameter of no more than 2.5' and would therefore appear starlike to the naked eye. At its brightest ("full moon") it would be about as bright as Venus is from Earth; at the first or third quarter phase it would be about as bright as Vega. When Deimos passes in front of the Sun its angular diameter is only about 2.5 times the angular diameter for Venus during a transit of Venus from Earth. With a small telescope, a Martian observer could see Deimos' phases, which take 1.2648 days to run their course (Deimos' synodic period).
Unlike Phobos, which orbits so fast that it actually rises in the west and sets in the east, Deimos rises in the east and sets in the west. However, the orbital period of Deimos of about 30.4 hours exceeds the Martian solar day ("sol") of about 24.7 hours by such a small amount that it takes 2.7 days between rising and setting for an equatorial observer.
Because Deimos' orbit is relatively close to Mars and has only a very small inclination to Mars' equator, it cannot be seen from Martian latitudes greater than 82.7°.
Deimos (oē-chheⁿ) | Деймос (спътник) | Deimos (satèl·lit) | Deimos (měsíc) | Deimos (måne) | Deimos (Mond) | Deimos (luna) | Dejmo | Déimos (lune) | Deimos (mjesec) | Deimos (luna) | דימוס (ירח) | Dimos (satelles) | Deimas (palydovas) | Deimos (maan) | ダイモス (衛星) | Deimos | Marsmånen Deimos | Deimos (księżyc) | Deimos | Деймос (спутник Марса) | Деимос | Deimos (mesiac) | Deimos (luna) | Deimos | Deimos (måne) | ดีมอส | Deimos (buwan) | Деймос (супутник) | 火卫二
This article is licensed under the GNU Free Documentation License.
It uses material from the
"Deimos (moon)".
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