Formation Flying
Higher angular resolution in astronomical images requires increasing apertures of telescopes or increasing baselines of interferometers. The mass of the support structure of the telescopes increases accordingly, and propellant for launch and navigation of long baseline space telescopes is about to exceed technical and financial boundaries. The revolutionary idea to overcome the mass constraint is to combine satellites in autonomous formation flight to behave just like a rigid body.
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Artist's impression of a formation flying space interferometer |
Autonomous Formation Flight is intended to allow satellites to fly in formation using advanced positioning and control loop technology. Multiple spacecraft configurations enable the formation to reconfigure, adapt baselines and acquire targets. Moreover, in case of failure of one satellite, it is easier to replace one of the spacecrafts during the mission instead of repairing a subsystem of a big assembly in space.
By now, ESA is implementing or assessing several space missions involving formation flight aspects:
| Mission Name |
Mass [kg] |
Projected launch year |
| LISA Pathfinder |
470 |
2008 |
| SWARM |
1000 |
2009 |
| PROBA-3 |
150 |
2009 |
| MAX |
200 |
2010 |
| XEUS |
tbd |
2015+ |
| NIRI (DARWIN) |
500 |
2015+ |
Last Update: 24 Feb 2006