Phobos has an anomalously low density. 1.876 g/cm^3.
In the late 1950s and 1960s, the unusual orbital characteristics of Phobos led to speculations that it might be hollow . The issue is still not settled – Phobos has a surface composition similar to that of carbonaceous chondrites, with spectra & albedo very similar to those of C- or D-type asteroids.
Ordinary chondrites (think of them as “rocks”) have densities of 3.2 to 3.4 g/cm^3.
Carbonaceous chondrites have densities of 2.1 to 3.4 g/cm^3.
So some of the interior of Phobos is probably empty space.
Mars Express is going in for the closest ever flyby of Phobos tomorrow (29/12/2013), just 45 km from the surface . It’s going to be so close that it can’t take pictures with its highest resolution camera. Instead, pictures have & will be taken on 21 Dec 2013 and 4 Jan 2014. The deflection of the track will be used, over the next few weeks, to find out what the gravity field of Phobos is like and to use this to probe the structure of Phobos’s interior for high and low density regions, to see if it’s a pile of rubble for example.
On the other hand, Phobos is far from being the asteroid with the lowest density . Asteroid 15 Eunomia may have a density as low as 0.96. 45 Eugenia has a density near 1.2. 90 Antiope and 253 Mathilde have densities near 1.3.
