Space is big, but not big enough

From the beginning of the space era, satellites and deep-space probes have populated the Solar System. There are now a huge number of satellites orbiting the Earth, for different purposes including Earth observation, weather forecasting, telecommunications, military applications, and astronomy. The space around Earth is therefore becoming more and more crowded. Aside from the aspect of 'space traffic control', there is the question of what to do with space litter.

ESA's European Space Operations Centre (ESOC) in Darmstadt, Germany, tracks space litter. It estimates that over 23 000 objects larger than 10 centimetres have been launched from Earth. Of these, about 7500 are still orbiting - only a very small proportion of them (6%) is operational. Half of all the objects are inoperable satellites, spent rocket stages, or other large space litter; the remaining 44% is debris from explosions and accidents in space. To make things worse, there are an estimated 70 000 to 120 000 fragments smaller than 1 centimetre and the amount of space debris increases by about 5% every year.

Tiny fragments, such as paint flecks, moving at very high velocities of around 6 kilometres per second can create problems for the spacecraft and for astronaut. One way to lower the threat is to remove satellites from orbit at the end of their working lives. If we force satellites down through the Earth's atmosphere, they burn up. However, this is more complicated if the satellite is so large that parts of it are liable to survive reentry and strike the ground. This is the case for some Earth observation satellites, for example, which are very big and heavy. When removing a (dead) satellite from orbit is too difficult, it is simply left in orbit.

However ESA is developing a new technology for its Darwin mission. This technology may allow smaller, more easily disposable satellites to replace often enormous relics in the future and may improve spacecraft control.

Darwin will use a flotilla of six 2-metre-diameter telescopes, flying in tight formation, to simulate a single telescope up to 250 metres across. The new technology being developed for Darwin allows the flotilla of spacecraft to control their mutual position with extremely high accuracy. In the case of Darwin, this enables you to analyse the atmospheres of very far-away Earth-like planets with high precision and detect the chemical signatures of life. Once this technology is developed, this could also find other applications: miniaturised versions of such technology could replace large, traditional satellites. "Imagine using an array of 20-centimetre telescopes. They would be small, light and easy to mass-produce, so cheap to manufacture," says Malcolm Fridlund, ESA's Project Scientist for the Darwin mission. They would see objects just as sharply as traditional satellites, if not better, and, at the end of their mission, scientists could ensure that they burn up in Earth's atmosphere like shooting stars. This way we keep space cleaner.

Another improvement is to position satellites further away, to reduce 'traffic jams' in near-Earth space. "This is a better position for Earth observation anyway," says Fridlund, "Because in low-Earth-orbit the satellite orbits every 90 minutes, it is only over each spot on Earth for a short period of time. In geostationary orbit, however, the satellite would be looking at one whole hemisphere continuously, so you could just point the array to wherever you are interested." Moreover, we could use Darwin's formation-flying technology to equip every satellite with a collision-avoidance system. Unrelated satellites would communicate with their neighbours and take corrective action if they began to drift together.

Of course, nothing will completely remove the threat of space litter. However, if we can use advanced technology to remove unwanted hardware from orbit, space will definitely become safer.