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ESA released new images of Mars’ moon Phobos, taken during the Mars Express March 7, 2010 flyby, showing the rocky moon in exquisite detail and also in 3-D. Mars Express orbits the Red Planet in a highly elliptical, polar orbit that brings it close to Phobos every five months, and it is the only spacecraft currently in orbit around Mars whose orbit reaches far enough from the planet to provide a close-up view of Phobos. Like our Moon, Phobos always shows the same side to the planet, so only by flying outside the orbit is it possible to observe the moon’s far side. Mars Express did such flybys on March 7, 10 and 13. Get out your 3-D glasses for a great look at Phobos, below.
Phobos is an irregular body measuring some 27 × 22 × 19 km. Its origin is debated. It appears to share many surface characteristics with the class of ‘carbonaceous C-type’ asteroids, which suggests it might have been captured by Mars. However, it is difficult to explain either the capture mechanism or the subsequent evolution of the orbit into the equatorial plane of Mars. An alternative hypothesis is that it formed around Mars, and is therefore a remnant from the planetary formation period.
In 2011 Russia will send a mission called Phobos–Grunt (meaning Phobos Soil) to land on Phobos, and an experiment will collect a soil sample and return it to Earth for analysis.
Phobos-Grunt will also carry with it The Planetary Society’s LIFE experiment which will test the survivability of microorganisms in the conditions of deep space. The experiment is a study of the panspermia hypothesis, which posits that microorganisms have traveled between planets sheltered deep inside space rocks.
For operational and landing safety reasons, the proposed landing sites were selected on the far side of Phobos within the area 5°S-5°N, 230-235°E. But new HRSC images showing the vicinity of the landing with better illumination from the Sun that previous images, which will provide valuable views and information for mission planners.
Mars Express will continue to encounter Phobos until the end of March, when the moon will pass out of range. During the remaining flybys, the high-resolution camera and other instruments will continue to collect data.
Source: ESA