Phobos

Mars I

        orbit:    9378 km from the center of Mars
        diameter: 22.2 km (27 x 21.6 x 18.8)
        mass:     1.08e16 kg

   Discovered 1877 August 12 by Hall; photographed by Mariner 9 in 1971, Viking 1 in 1977, and Phobos in 1988.

   Phobos orbits Mars below the synchronous orbit radius. Thus it rises in the west, moves very rapidly across the sky and sets in the east, usually twice a day. It is so close to the surface that it cannot be seen above the horizon from all points on the surface of Mars.

   And Phobos is doomed: because its orbit is below synchronous altitude tidal forces are lowering its orbit (current rate: about 1.8 meters per century). In about 50 million years it will either crash onto the surface of Mars or (more likely) break up into a ring. (This is the opposite effect to that operating to raise the orbit of the Moon.)

   Phobos and Deimos may be composed of carbon-rich rock like C-type asteroids. But their densities are so low that they cannot be pure rock. They are more likely composed of a mixture of rock and ice. Both are heavily cratered. New images from Mars Global Surveyor indicate the Phobos is covered with a layer of fine dust about a meter thick, similar to the regolith on the Earth's Moon.

   The Soviet spacecraft Phobos 2 detected a faint but steady outgassing from Phobos. Unfortunately, Phobos 2 died before it could determine the nature of the material; water is the best bet. Phobos 2 also returned a few images (right).

   The most prominent feature on Phobos is the large crater named Stickney, the maiden name of Hall's wife (above). Like Mimas' crater Herschel (on a smaller scale) the impact that created Stickney must have almost shattered Phobos. The grooves and streaks on the surface were probably also caused by the Stickney impact.

   Phobos and Deimos are widely believed to be captured asteroids. There is some speculation that they originated in the outer solar system rather than in the main asteroid belt.

   Phobos and Deimos may someday be useful as "space stations" from which to study Mars or as intermediate stops to and from the Martian surface; especially if the presence of ice is confirmed.

More about Phobos

• more images
• from LANL

Open Issues

• It seems likely that Phobos and Deimos formed elsewhere and subsequently captured by Mars. But how did the capture occur? Was it made possible by a thicker Martian atmosphere long ago?