Phoebe is a peculiar moon
amongst the 31 known satellites orbiting Saturn. Most of Saturn's moons are
bright but Phoebe is very dark and reflects only 6% of the Sun's light.
Another difference is that Phoebe revolves around the planet on a rather
elongated orbit and in a direction opposite to that of the other large moons
(a motion known as 'retrograde' orbit).
All these hints suggested that Phoebe, rather
than forming together with Saturn, was captured at a later stage. Scientists,
however, do not know whether Phoebe was originally an asteroid or an object
from the 'Kuiper Belt', a region of comets and other small, icy objects at the
fringes of the Solar System.
The images obtained by
Cassini's high-resolution camera now seem to indicate that it contains
ice-rich material and is covered by a thin layer of dark material, probably
300-500 metres thick.
Scientists base this hypothesis on the
observation of bright streaks in the rims of the largest craters, bright rays
radiating from smaller craters, grooves running continuously across the
surface of the moon and, most importantly, the presence of layers of dark
material at the top of crater walls.
"The imaging team is
in hot debate at the moment on the interpretations of our findings," said
Dr Carolyn Porco, Cassini imaging team leader at the Space Science Institute
in Boulder, USA.
"Based on our images, some of us are
leaning towards the view that has been promoted recently, that Phoebe is
probably ice-rich and may be an object originating in the outer solar system,
more related to comets and Kuiper Belt objects than to asteroids."
The high-resolution images of Phoebe show a
world of dramatic landforms, with landslides and linear structures such as
grooves, ridges and chains of pits. Craters are ubiquitous, with many smaller
than one kilometre.
"This means, besides the big ones, lots of
projectiles smaller than 100 metres must have hit Phoebe," said Prof.
Gerhard Neukum, Freie Universitaet Berlin, Germany, and a member of the
imaging team. Whether these projectiles came from outside or within the Saturn
system is debatable.
There is a suspicion that Phoebe, the largest
of Saturn's outer moons, might be parent to the other, much smaller retrograde
outer moons that orbit Saturn. They could have resulted from the impact ejecta
that formed the many craters on Phoebe.
Besides these stunning images, the instruments
on board Cassini collected a wealth of other data, which will allow scientists
to study the surface structures, determine the mass and composition of Phoebe
and create a global map of it.
"If these additional data confirm that
Phoebe is mostly ice, covered by layers of dust, this could mean that we are
looking at a 'leftover' from the formation of the Solar System about 4600
million years ago," said Dr Jean-Pierre Lebreton, ESA Huygens Project
Scientist.
Phoebe might indeed be an icy wanderer from the
distant outer reaches of the Solar System, which, like a comet, was dislodged
from the Kuiper Belt and captured by Saturn when the planet was forming.
Whilst studying the nature of Phoebe may give
scientists clues on the origin of the building blocks of the Solar System,
more data are needed to reconstruct the history of our own neighbourhood in
space.
With that aim, ESA's Rosetta mission is on its
way to study one of these primitive objects, Comet 67P/Churyumov-Gerasimenko,
from close quarters for over a year and land a probe on it.
The fly-by of Phoebe on 11 June was the only
one that Cassini-Huygens will perform with this mysterious moon. The mission
will now take the spacecraft to its closest approach to Saturn on 1 July, when
it will enter into orbit around the planet.
From there, it will conduct 76 orbits of Saturn
over four years and execute 52 close encounters with seven other Saturnian
moons. Of these, 45 will be with the largest and most interesting one, Titan.
On 25 December, Cassini will release the Huygens probe, which will descend
through Titan's thick atmosphere to investigate its composition and complex
organic chemistry.