Phobos flyby success

Mar 04, 2010
This image of Phobos's surface was obtained by the Super Resolution Channel (or SRC, a part of the High Resolution Stereo Camera experiment) on board ESA's Mars Express onAug. 3, 2008 (orbit 5889). The distance from the moon's centre was 656 km, and the image resolution is 6 m/pixel. The original image has been corrected for mirror distortion. Credit: ESA/ DLR/ FU Berlin (G. Neukum)

Mars Express encountered Phobos last night, smoothly skimming past at just 67 km, the closest any manmade object has ever approached Mars' enigmatic moon. The data collected could help unlock the origin of not just Phobos but other 'second generation' moons.

Something is not right about . It looks like a solid object but previous flybys have shown that it is not dense enough to be solid all the way through. Instead, it must be 25-35% porous. This has led planetary scientists to believe that it is little more than a 'rubble pile' circling Mars. Such a rubble pile would be composed of blocks both large and small resting together, with possibly large spaces between them where they do not fit easily together.

Last night's flyby was close enough to give scientists their most exquisite data yet about the of Phobos. Mars Express locked onto the radio signal from Earth at around 21:20 CET (20:20 UT). The radio frequency oscillators on the ground are 100 000 times more stable than those on the spacecraft, so for this experiment, which required the best precision possible, the signal was sent up to Mars Express and then returned by the spacecraft to the ground.

The radio waves travel at the speed of light and took 6 minutes 34 seconds to travel from Earth to the last night. So the round trip time was 13 minutes 8 seconds. Once the signal was received back at Earth, it was clearly strong and good. So strong that radio amateurs were also able to lock onto the signal, although their equipment would not be able to detect the subtle variations induced by the of Phobos.

Now that the data are all collected, the analysis can begin. First will be an estimate of the density variation across the moon. This will tell scientists just how much of Phobos' interior is likely to be composed of voids.

"Phobos is probably a second-generation Solar System object," says Martin Pätzold, Universitat Koln, Cologne, Germany, and Principal Investigator of the Mars Radio Science (MaRS) experiment. Second generation means that it coalesced in orbit after Mars formed, rather than forming concurrently out of the same birth cloud as the Red Planet. There are other moons around other planets where this is thought to have been the case too, such as Amalthea around Jupiter.

Whatever the precise origin, Phobos will eventually crumble back into this disrupted state. It is gradually spiralling towards Mars and will eventually be pulled apart. "It came from debris, it will return to debris," says Pätzold. In the meantime, it is there to be studied and explored.

Last night's was just one of a campaign of 12 Mars Express flybys taking place in February and March 2010. For the previous two, the radar was working, attempting to probe beneath the surface of the moon, looking for reflections from structures inside. In the coming flybys, the camera will take over, providing high resolution pictures of the moon's surface.

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Caliban
3.5 / 5 (6) Mar 04, 2010
Hmmm
What's the deal with all the banding/striation? Evidence of stratification? Seems unlikely that these are tracks plowed through a dusty, granular surface, if only because of their persistence over such large distances. Also, you would expect that if it formed by acretion, it would have been built- so to speak- from the inside out, rather than as some type of horizontally oriented "strata".
Just speculating.
malapropism
4.3 / 5 (3) Mar 04, 2010
And in addition, it's clear from this image that at least some of the craters occurred after the striations, perhaps implying that the banding is an early artifact. It would be interesting to see more photographic coverage to see how extensive this striation is over the whole body of the moon. If a striation "layer" could be traced all the way around (possibly indicating it also goes all the way through since I can't conceive of something that might make marks like those around the surface - planetary sized snail trails, maybe?), might this imply that the whole thing is a lump that was originally sedimented?
Caliban
2.5 / 5 (4) Mar 04, 2010
I wondered the same. But how to get that size chunk ejected from a planetary surface, and then into orbit around Mars? Would've had to have come from a relatively evolved planet, too. Mercury, Venus, Earth, Mars- extrasolar, even. I noticed, too, that the "striations" seem to follow the surface contours, as well, which would seem to indicate that they are structural.
zuggerjack
4 / 5 (2) Mar 05, 2010
Yes, those intricate striations demand further investigation, preferably on-site manned analysis. Landing two geologist-astronauts on Phobos should be at the top of the White House space agenda, as recommended by David Kagan, US aerospace engineer and author of the book Sunstroke. I agree with Kagan, and many astronomers who believe Phobos was originally an asteroid that was captured by Mars' gravity. A crewed mission to Phobos would serve two practical purposes: getting humanity way out of low-earth-orbit to another planet's gravity environment and, if Phobos is indeed an asteroid, such a mission would help determine the best way to divert one of these giant space rocks from hitting Earth.

Putting astronauts on Phobos is infinitely easier than a manned landing on Mars due to this moon's minor gravity field, and Lockheed-Martin Corp. can do it in ten years, under NASA's supervision.