Phobos
Mars I
Phobos Facts
- Phobos is the larger and innermost of Mars's two moons:
- distance from (the center of) Mars: 9378 km
- diameter: 22.2 km (27 x 21.6 x 18.8)
- mass: 1.08e16 kg
Phobos is closer to its primary than any other moon in the Solar System,
less than 6000 km above the surface of Mars; it
is also one of the smallest moons
in the solar system.
- Pronounced "FOH bus"
- In Greek mythology, Phobos is one of the sons of Ares (Mars) and
Aphrodite (Venus).
"phobos" is Greek for "fear" (the root of "phobia").
- Discovered 1877 August 12
by Hall, photographed by
Viking 1 in 1977.
- Phobos orbits Mars below the
synchronous orbit radius. 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.
- Phobos is doomed: because its orbit is below synchronous altitude
tidal forces are pulling it toward Mars. In less than
100 million years it will either break up into a
ring or crash onto the surface of Mars.
- Phobos and Deimos may be composed of carbon-rich
rock like C-type asteroids.
But their densities are so low that cannot be pure rock. They are more
likely composed of a mixture of rock and ice.
Both are heavily cratered.
- 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.
- The most prominent feature on Phobos is the large crater named Stickney
(the maiden name of A. Hall's wife).
Like Mimas's 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.
Pictures
- (above) Phobos's crater Stickney
21k jpg;
143k gif
- another view of Stickney
121k gif;
26k jpg
the other side
35k gif
- Map of Phobos
163k gif
- Phobos, Deimos, Gaspra and Ida compared
96k jpg
- Close up
17k gif
- Close up
11k gif
- Close up
13k gif
Close up
17k gif
- Close up
18k gif
More about Phobos
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
atmosphere long ago?
... Mars
... Phobos
... Deimos
...
Bill Arnett; last updated:
1995 June 12