Deimos the smaller Mar’s moon is 9 miles across its width and Phobos is 17 miles across its width. It has a large crater named stickney on its surface which ia about 3 miles across.
In the 60’s and 70’s, the Mariner and Vikings space probes sent back detailed pictures of the surface of Mars. The most recent successful Mars missions called Mars Pathfinder and Mars Global Surveyor were launched in 1996. The Surveyor craft was use for sending images and information from Mars. The vehicle carried by the Pathfinder is named Sojourner. This vehicle roamed over Mars planet’s surface taken photographs and performing certained programmed studies which were transmitted into earth.
Another hypothesis is that Mars was once surrounded by many Phobos- and Deimos-sized bodies, perhaps ejected into orbit around it by a collision with a large planetesimal. The high porosity of the interior of Phobos (based on the density of 1.88 g/cm3, voids are estimated to comprise 25 to 35 percent of Phobos’ volume) is inconsistent with an asteroidal origin. Observations of Phobos in the thermal infrared suggest a composition containing mainly phyllosilicates, which are well known from the surface of Mars. The spectra are distinct from those of all classes of chondrite meteorites, again pointing away from an asteroidal origin. Both sets of findings support an origin of Phobos from material ejected by an impact on Mars that reacted in Martian orbit, similar to the prevailing theory for the origin of Earth’s moon.
The motions of Phobos and Deimos would appear very different from that of our own Moon. Speedy Phobos rises in the west, sets in the east, and rises again in just eleven hours, while Deimos, being only just outside synchronous orbit, rises as expected in the east but very slowly. Despite its 30 hour orbit, it takes 2.7 days to set in the west as it slowly falls behind the rotation of Mars, and has long again to rise.
Both moons are tidally locked, always presenting the same face towards Mars. Since Phobos orbits Mars faster than the planet itself rotates, tidal forces are slowly but steadily decreasing its orbital radius. At some point in the future, when it approaches Mars closely enough, Phobos will be broken up by these tidal forces. Several strings of craters on the Martian surface, inclined further from the equator the older they become, suggesting that, there may have been other small moons that suffered the fate expected of Phobos, and also that the Martian crust as a whole shifted between these events. Deimos, on the other hand, is far enough, away that its orbit is being slowly boosted instead of, as in the case of the earth’s Moon.