The “groovy” martian moon

Europe's Mars Express returns its first close-up images of Phobos.
By | Published: November 12, 2004
Mars Express images Phobos
Phobos, the largest martian moon, was gouged and nearly shattered by the impact that formed its 6-mile-wide (10 kilometer) Stickney, its largest crater. Mars Express was less then 125 miles (200 km) away August, 22, 2004, when it took this image of the moon’s Mars-facing side.
ESA / DLR / FU Berlin (G. Neukum)
Phobos in 3D
Mars Express scientists generated this anaglyph 3-D view of Phobos, but you’ll need red-blue stereo glasses to see the effect.
ESA / DLR / FU Berlin (G. Neukum)
Boulder on Phobos
A large boulder casts a stark shadow across Phobos’ bleak landscape. The rock, probably ejected by the Stickney impact, is about 280 feet (85m) wide. Mars Global Surveyor captured the images during its September 16, 1998 flyby.
NASA / JPL / Malin Space Science Systems
Stickney up close
The formation of Stickney Crater, which is nearly half the size of Phobos, may have come close to tearing the moon apart. The prominent grooves are shallow, elongated depressions that may be fractures from the Stickney impact. Individual boulders more than 160 feet (50 meters) wide can be seen on the crater’s near rim in this image from Mars Global Surveyor, which flew past Phobos on August 19, 1998.
NASA / JPL / Malin Space Science Systems
November 12, 2004
Named for fear itself, Phobos, the largest and innermost of the two martian moons, bears a disarming resemblance to a striated potato. Scientists hope new views from the European Space Agency’s (ESA) Mars Express spacecraft will shed light on how it got that way.

Phobos, which orbits Mars 3 times a day, is an elliptical body about 17 by 11 miles (27 by 18 kilometers) in size. Its most striking features are a single impact crater nearly half the moon’s size, and a puzzling, global network of grooves. Many think the two are related because the formation of the 6-mile-wide (10 km) crater, named Stickney, probably came close to shattering the moon.

When Mars Express periodically makes a close approach to Phobos, the spacecraft turns away from the Red Planet and trains its High Resolution Stereo Camera (HRSC) on the martian moon. Since entering Mars orbit December 25, 2003, the probe has whisked past Phobos 6 times, returning images with ever-greater resolution. The probe’s most recent pass, August 22, 2004, brought it within 175 miles (200 km) of the moon.

Mars Express shot 10 different images of Phobos at nearly the same time — among the most detailed views ever seen. They cover more of the moon’s illuminated surface than those of previous missions, plus the best pictures aren’t blurred by spacecraft motion, a problem with some high-resolution images from other missions.

Because the same side of Phobos always faces the Red Planet, Mars Express images show only that hemisphere. Crater walls on the moon show dark streaks from landslides, proof that gravity just 1/1000th that of Earth’s shapes the terrain. On Phobos, a 150-pound (68 kilogram) person would weigh only 2 ounces (57 grams).

Although Phobos appears bright in spacecraft images, it reflects only about 6 percent of the light it receives — little better than a freshly paved parking lot. In fact, the dark surfaces of Phobos and the outer martian moon, Deimos, lead scientists to suspect kinship with carbonaceous-chondrite asteroids. Both moons may have been wayward asteroids captured into orbit around the Red Planet.

Phobos appears to be nearing Mars by 6 feet (1.8 meters) every century, a rate that will crash it into Mars some 50 million years from now. But the little, fractured moon may not even survive to reach the surface. As Phobos nears the planet, martian tides may succeed where the Stickney impact failed — they may destroy the moon. If so, future astronomers will witness the moon’s transformation from a dark satellite to a bright new ring of rock and dust.