Posted by Emily Lakdawalla
2007/08/17 12:44 CDT
The MESSENGER spacecraft is headed toward its first of three flybys of Mercury, on January 14, 2008. (It will take three flybys to match its orbital geometry close enough to Mercury's so that it will be able to enter Mercury orbit on March 18, 2011.) It is now in a pretty tight orbit around the Sun, and on September 1, it will reach its closest perihelion yet, passing through a minimum distance to the Sun of only 0.33 Astronomical Units. Being three times closer to the Sun than Earth means that the Sun now feels nine times stronger to MESSENGER than it does to the Earth-orbiting spacecraft that MESSENGER left behind three years ago.
Louise Prockter is an outer planets scientist who's also working on the MESSENGER MDIS camera team, and during the conference she invited me to take a look at a preliminary imaging plan for the January flyby. The three-flyby plan is strangely similar to the mission of Mariner 10, which flew by Mercury three times in 1974 and 1975. Because of Mercury's spin-orbit resonance, Mariner 10 saw the same hemisphere, with pretty much the same lighting geometry, on all three encounters, which means that fully half of Mercury has never been seen by spacecraft. MESSENGER, too, will see the same hemisphere sunlit on all three of its flybys, but whether due to good fortune or good planning or some combination of the two, the MESSENGER hemisphere will be almost exactly that side of Mercury that was not seen by Mariner 10.For the January flyby, MESSENGER will approach somewhat from behind Mercury, seeing mostly territory previously viewed by Mariner 10 at a high phase angle (so Mercury will appear as a crescent). There is a three-color approach movie planned, which will show Mercury's crescent gradually swelling in to view. The imaging has to be fit in around the activities of MESSENGER's other science instruments, particularly the spectrometer, MASCS, which will be very active on approach, swinging back and forth to map the planet's composition. Closest approach will occur over Mercury's night side, which is a bit of a bummer for imaging, but it's wonderful for MESSENGER's laser altimeter instrument, MLA. The animation that Louise showed me included hundreds of shots of MLA firing at the surface, gathering a detailed topographic profile, the first of its kind for Mercury. I'm not sure what kind of resolution it will have, or what sort of terrain it will cross. After the close approach, the gods of orbital mechanics smile upon the camera. The geometry of planet and Sun require MESSENGER to point its sunshade in such a direction that all but one of the instruments pretty much can't be used after closest approach. The exception is MDIS, the camera, which has its own pivot, so it can point at Mercury when the other instruments cannot. So MDIS pretty much has the entire post-flyby time to itself; and right after the flyby is when Mercury will present the previously unseen face to the camera, at relatively low phase, meaning that most of the globe will be sunlit. The animation that Louise showed me basically had MDIS scanning across Mercury like a typewriter, shooting a frame, moving one frame to the right, shooting a frame, and so on for 10 frames or so, then doing a carriage return and starting the next line of frames, building up an enormous high-resolution monochrome mosaic at very high speed. (I asked why the carriage return, and she said that they looked at different ways of building mosaics, and the geometry works out better with the carriage return instead of whisking back and forth.)
The post-flyby sequence starts with the highest-resolution mosaic centered on the equator, then as MESSENGER recedes, it shoots full-planet mosaics. After receding a bit more the imaging switches to color views; flash-flash-flash, MDIS grabs 11 images of the same spot through each of its color filters before moving to the next spot. And, because none of the other instruments can operate, every time MDIS finishes a global mosaic, it starts over with another one. Louise told me that they want to make absolutely totally sure they get this view of the unseen side; it's one of their major mission success criteria, and one they can accomplish long before they go into orbit. She said she didn't know how many of the mosaics they'd really be able to do, but they'll do as many as data volume allows. At some point they switch from shooting global mosaics to a narrow-angle, single-color movie of the departure; it will start with Mercury more than filling the field of view, and end with it appearing as a small ball in the center.
Louise says that the current plan is for the radio science team to be "doing something" for the couple of days following the encounter, so image data won't start returning to Earth until after that, and that the order in which it will be returned has something to do with the compression being performed onboard the spacecraft.
That hemisphere of Mercury is, I think, the largest surface in the solar system that hasn't been seen by a spacecraft (at 5,000 kilometers in diameter, half of Mercury is actually bigger than, say, all of Pluto or Eris, which are about 2,300 and 2,400 kilometers in diameter, respectively). However, I should point out that that hemisphere isn't actually completely unknown. Far from it, in fact. Here's a recent map that combines the Mariner 10 data with radar images produced by Arecibo.
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