Abstract :
The cathode-less electron cyclotron resonance ion engines, μ10, propelled the Hayabusa asteroid explorer, launched in May 2003, which is focused on demonstrating the technology necessary for a sample return from an asteroid, using electric propulsion, optical navigation, material sampling in a zero gravity field, and direct re-entry from a heliocentric orbit. It rendezvoused with the asteroid Itokawa after a two-year deep space flight using the ion engines. Though it succeeded in landing on the asteroid on November 2005, the spacecraft was seriously damaged. This delayed Earth return in 2010 from the original plan in 2007. Reconstruction on the operational scheme using thrust vector control of ion engines, Xe cold gas jets and solar pressure torque made Hayabusa leave for Earth in April 2007. Although most of the neutralizers were degraded and unable to be used in fall of 2009, a combination of an ion source and its neighboring neutralizer has kept the orbit maneuver to Earth including a series of final trajectory correction maneuvers. Finally, the spacecraft decayed in atmosphere and only the reentry capsule was retrieved from the Australian outback on June 14th, 2010. For the round trip space odyssey between Earth and the asteroid, the ion engines served the total accumulated operational time 39,637 hour·unit, the powered spaceflight in 25,590 hours, delta-V of 2.2 km/s, total impulse of 1 MN·s and 47 kg Xenon propellant consumption.
Keywords :
aerospace instrumentation; asteroids; astronomical instruments; celestial mechanics; space vehicles; Hayabusa asteroid explorer; Itokawa asteroid; Xe cold gas jets; Xenon propellant consumption; cathode-less electron cyclotron resonance ion engines; deep space flight; electric propulsion; heliocentric orbit; material sampling; optical navigation; round trip space odyssey; solar pressure torque; spaceflight; thrust vector control; zero gravity field; Earth; Engines; Orbits; Propulsion; Space vehicles; Sun; Torque;