The Martian Moons![]()
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Mars has two moons, Phobos [FOH-bohs] (above left) and
Deimos [DEE-mos] (above right) These are extremely small moons (Phobos being
the larger of the two) that have extremely fast orbital periods. Phobos
(fear) and Deimos (panic) were named after attendants of the Roman god of
War, Mars.
Their surface compositions
are similar to the C-type (blackish carbonaceous chondrite) asteroids that
exist in the asteroid belt that lies beyond Mars . While some scientists
speculate that Phobos and Deimos are captured asteroids, other scientists
point to evidence that contradicts this theory. Both Deimos and Phobos are
covered with craters. Deimos has a smoother appearance caused by partial
filling of some of its craters. Phobos shows striated patterns which are
probably cracks caused by the impact event which created the largest crater
on the moon. On the left is an image of Deimos taken by the Mars Pathfinder
Lander.
Deimos Statistics
| Discovered by | Asaph Hall |
| Date of discovery | 1877 |
| Mass (kg) | 1,800,000,000,000,000. |
| Length (km) | 15 km long |
| Mean distance from Mars (km) | 23,460 |
| Rotational period (days) | 1.26244 |
| Orbital period (days) | 1.26244 |
| Radius (Earth = 1) | 0.0001759 |
| Mean density (gm/cubic cm) | 1.7 |
Phobos Statistics
| Discovered by | Asaph Hall |
| Date of discovery | 1877 |
| Mass (kg) | 10,800,000,000,000,000. |
| Length (km) | 27 km long |
| Mean distance from Mars (km) | 9,380 |
| Rotational period (days) | 0.31910 |
| Orbital period (days) | 0.31910 |
| Radius (Earth = 1) | 0.0021167 |
| Mean density (gm/cubic cm) | 2.0 |