Hayabusa, like many other spacecraft, possesses three reaction wheels, oriented 90° to one another. It had already lost one — the x-axis reaction wheel — July 31; the y-axis reaction wheel failed October 2. This means the probe has to maintain its orientation using just the z-axis reaction wheel and its thrusters, which will consume valuable fuel.
Mission managers are assessing the consequences of these technical hardships for the mission and studying ways to minimize fuel use. They remain optimistic that Hayabusa will be able to accomplish its primary tasks of dropping off Minerva and capturing a small piece of Itokawa's surface.
The spacecraft has already nearly completed its mapping of Itokawa. The images contain many puzzles. Sho Sasaki, in a presentation at last week's Dust in Planetary Systems conference in Hawaii, showed pictures of smooth and rough areas, some containing boulders many yards (meters) in diameter. The presence of large boulders on the surface suggests the asteroid's interior may be a loosely held "rubble pile."
Scientists speculate Itokawa's strange shape may be the result of a collision between two smaller asteroids, which fused into the 1,650-foot-wide (500m) asteroid observed today. A smooth area, tentatively dubbed the "Muses Sea" by mission scientists, may mark the area of contact. (The name plays off the mission's original name, MUSES-C.)
Mission planners currently expect to choose a landing site in mid-October. Approximately 1 month later, Hayabusa is slated to descend to the asteroid's surface, collect a small sample, and drop off Minerva. Then, in December, the spacecraft will depart Itokawa, and return pieces of the asteroid to Earth in June 2007.Bill Cooke is an astronomer with NASA's Marshall Space Flight Center in Huntsville, Alabama.