Phobos is what scientists call a ‘small irregular body’. Measuring 27 km × 22 km × 19 km, it is one of the least reflective objects in the Solar System, thought to be a capture-asteroid or a remnant of the material that formed the planets.
The best images of Phobos ever
The HRSC images, which are still under processing, form a bounty for scientists studying Phobos. They are a result of observations carried out over several close fly-bys of the martian moon, performed over the past three weeks. At their best, the pictures have a resolution of 3.7 m/pixel and are taken in five channels (in the stereo channel) for images in 3-D and (in the photometric channels) to perform analyses of the physical properties of the surface.
The images obtained by several other spacecraft so far have either been of a lower resolution, or not available in 3D and have not covered the entire disc of Phobos. This is also the first time that portions of the far-side of the moon have been imaged in such high resolution (Phobos always faces Mars on the same side).
In observing Phobos, Mars Express benefits from its highly elliptical orbit which takes it from a closest distance of 270 km from the planet to a maximum of 10 000 km (from the centre of Mars), crossing the 9000 km orbit of the martian moon. Mars Express imaged the far-side of Phobos (with respect to Mars) for the first time after NASA’s Viking mission, by flying outside the spacecraft’s orbit around Mars.
Phobos-Grunt (Phobos soil), a Russian sample-return mission, is due to for launch in 2009. It is expected to land on the far-side of Phobos at a region between 5° south to 5° north, and 230° west to 235° west. This region was last imaged in the 1970s by the Viking orbiters.
The HRSC observations have been awaited eagerly to better assess and characterise the choice of the landing site.
The moon's remarkably grooved surface can be seen in the pictures quite clearly. The origin of these grooves is still debated. It is not known whether they are produced by ejecta thrown up from impacts on Mars, or if they result from the surface regolith, or soil, slipping into internal fissures.
In this image, at least two families of grooves with distinct orientations can be seen along with an elongated crater.
The stereo observations (resolution 3.7 m/pixel) are important for structural analysis and they will be used to derive a digital terrain model (a 3-D map of the surface that includes elevation data). The extra photometric channels (at 7.4 m/pixel) make it possible to study the properties of the Phobos regolith at micron to millimetre scales.
An operational challenge
Managing the close fly-bys was an operational challenge, made possible by spacecraft operations engineers and scientists who worked together to specially optimise Mars Express’s trajectory and obtain the best possible views.
The observation made use of a spacecraft slew, a special manoeuvre whereby the body of the spacecraft is rotated against the direction of motion, to effectively lower the speed at which the target passes in the field of view of the camera. This makes it possible to avoid blurring of the pictures despite the high fly-by velocities, whilst maintaining acceptable exposure time.
The HRSC Super Resolution Channel (SRC) also observed during this close fly-by, with a nominal resolution of 90 cm/pixel. As expected, despite the slew, some residual motion blur has crept into the image, but much detail is expected to be recovered after further processing.
In the days running up to the observation, the primary star-tracker - a navigation device that helps the spacecraft point its instruments at the target accurately - experienced some temporary difficulty in recognising the star constellations in its field of view, leaving the spacecraft operating on its secondary system. Concerned that this might affect this critical observation, the team at ESA's European Space Operations Centre (ESOC) in Darmstadt, Germany, worked intensely to recover the primary system and were able to switch back successfully two days before the fly-by.
Agustin Chicarro | alfa
Ultra-compact phase modulators based on graphene plasmons
27.06.2017 | ICFO-The Institute of Photonic Sciences
Smooth propagation of spin waves using gold
26.06.2017 | Toyohashi University of Technology
19.06.2017 | Event News
13.06.2017 | Event News
13.06.2017 | Event News
27.06.2017 | Power and Electrical Engineering
27.06.2017 | Information Technology
27.06.2017 | Physics and Astronomy