During additional flybys of Deimos planned for later this year, “we’re going to get to around 200 kilometers [124 miles], and that’s still pretty good data,” she says. “That will help us understand the moon.”
Are Phobos and Deimos captured asteroids?
The mission to take the new photos of Deimos, with Mars looming large in the background, allowed the probe’s two spectrometers to record crucial data about the moon’s composition.
These initial readings are preliminary and will be refined in later flybys. But they suggest Deimos is made of rocky material similar to Mars itself, and not the carbon-rich rock that would be expected if Deimos was a captured asteroid, as scientists once suspected.
That supports theories that both Deimos and Phobos — Mars’ larger moon, which is nearly 17 miles (27 km) across at its widest point — formed in orbit when a large object, perhaps a dwarf planet, struck Mars in the distant past. If confirmed, that would put to rest long-standing theories that both Phobos and Deimos are asteroids that have been captured by Mars’ gravity.
But many questions remain, including whether Phobos has the same composition as Deimos. Both Martian moons are also small and irregularly shaped, which supports the idea they are captured asteroids; and both are optically very dark, unlike Mars itself, which suggests they may have a different origin than the Red Planet.
Understanding the origins of Phobos and Deimos