Russia’s Obsession with Mar’s Mystery Moon, Phobos -Destination of Planned Space Mission

Phobos One of the least reflective bodies in the solar system, Mars's largest moon, Phobos, orbits the planet below the synchronous orbit radius (it moves around Mars faster than the planet itself rotates). This image was taken by the European Space Agency's Mars Express — a spacecraft that has been circling Mars since Christmas 2003.

The probe recorded the images during a fly-by just 100 kilometres away on January 9, 2011. The circles mark the previously planned (red) and currently considered (blue) landing sites for the Russian Phobos-Grunt mission.

In a recent development, scientists say they have uncovered firm evidence that Phobos, is made from rocks blasted off the Martian surface in a catastrophic event, solving  a long-standing puzzle. It has been suggested that both Phobos and Deimos could be asteroids that formed in the main asteroid belt and were then "captured" by Mars's gravity.

An alternative theory suggests that Phobos could have been formed from the remnants of an earlier moon destroyed by Mars's gravitational forces. However, this moon might itself have originated from material thrown into orbit from the Martian surface.

Previous observations of Phobos at visible and near-infrared wavelengths have been interpreted to suggest the possible presence of carbonaceous chondrites, found in meteorites that have crashed to Earth. This carbon-rich, rocky material, left over from the formation of the Solar System, is thought to originate in asteroids from the so-called "main belt" between Mars and Jupiter.

New data from the European Space Agency's Mars Express spacecraft appears to make the asteroid-capture scenario look less likely. Recent observations — as thermal infrared wavelengths using the Planetary Fourier Spectrometer (PFS) instrument on Mars Express show a poor match between the rocks on Phobos and any class of chondritic meteorite known from Earth — seem to support the "re-accretion" models for the formation of Phobos, in which rocks from the surface of the Red Planet are blasted into Martian orbit to later clump and form Phobos.

"We detected for the first time a type of mineral called phyllosilicates on the surface of Phobos, particularly in the areas northeast of Stickney, its largest impact crater," said co-author Dr. Marco Giuranna, from the Italian National Institute for Astrophysics in Rome. These phyllosilicate rocks are thought to form in the presence of water, and have been found previously on Mars.

"This is very intriguing as it implies the interaction of silicate materials with liquid water on the parent body prior to incorporation into Phobos," said Dr Giuranna. "Alternatively, phyllosilicates may have formed in situ, but this would mean that Phobos required sufficient internal heating to enable liquid water to remain stable."

Other observations from Phobos appear to match the types of minerals identified on the surface of Mars. Thus, the make-up of Phobos appears more closely related to Mars than to asteroids from the main belt, say the researchers. In addition, said Pascal Rosenblatt of the Royal Observatory of Belgium, "the asteroid-capture scenarios also have difficulties in explaining the current near-circular and near-equatorial orbit of both Martian moons (Phobos and Deimos)".

The researchers also used Mars Express to obtain the most precise measurement yet of Phobos' density."This number is significantly lower than the density of meteoritic material associated with asteroids. It implies a sponge-like structure with voids making up 25%-45% in Phobos's interior," said Dr Rosenblatt. A highly porous asteroid would have probably not survived if captured by Mars. Alternatively, such a highly porous structure on Phobos could have resulted from the re-accretion of rocky blocks in Mars's orbit.

In describing the internal geometric structure of this "moon" as revealed by MARSIS,  European Space Agency (ESA) sources emphasized that "several of these interior Phobos compartments also appear to still be holding some kind of atmosphere … " which has given birth to wild speculation that Phobos could prove to be an artificial satellite of some sort.

The source repeated this several times . . . raising all kinds of fascinating questions regarding "how" the radar could, in fact, determine this — that some of the vast "rooms" inside Phobos ("from a quarter to half-a-mile in diameter . . .") were "maintaining an internal pressure."

Russia's robotic mission to Phobos, named Phobos-Grunt (grunt means ground, or earth, in Russian) to be launched in 2011, will investigate the moon's composition in more detail.


The Daily Galaxy via

Image shows Planned landing site of the Russian Phobos-Grunt mission
Image Credits: ESA/DLR/FU Berlin (G. Neukum)


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