How It Works

ORBITAL DEBRIS CAN MAKE A MESS OF THINGS

Our planet is surrounded by junk that poses a threat to astronauts and spacecraft

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Debris in space is a well-documented problem; NASA estimates that there are roughly 13,000 objects larger than ten centimetre­s in diameter floating around in the near-earth environmen­t. The danger from orbital garbage is all too apparent. In 1983, a tiny paint fleck hurtling through space hit Space Shuttle Challenger’s window, causing so much damage that the entire window had to be replaced. The Internatio­nal Space Station

(ISS) regularly manoeuvres out of the path of oncoming junk.

Most of this junk is moving at extremely high speeds – up to seven times the speed of a rifle bullet. At that speed, not only would you not see it coming, but an object no bigger than a penny could also easily destroy an aeroplanes­ized spacecraft. Although spacecraft are built with shielding to help protect them against this sort of collision, the risk of a major catastroph­e is on the increase.

Of even more concern is the prospect of ‘runaway’ disintegra­tion. This is known as the Kessler effect. If a major collision event were to occur in near-earth orbit, it could set off an uncontroll­able chain reaction, quickly resulting in large regions of space being awash with dangerous junk. Although the current levels of debris orbiting our planet are unlikely to present a high-level threat, this ‘critical mass’ could be achieved in only a few decades.

 ?? ?? hole A tiny chip of paint made this impact window of Space Shuttle Challenger in the
This NASA orbital debris plot shows primary debris fields in low-earth orbit, where 70 per cent of all catalogued debris is found. Another debris field can be found farther out in geosynchro­nous orbit
hole A tiny chip of paint made this impact window of Space Shuttle Challenger in the This NASA orbital debris plot shows primary debris fields in low-earth orbit, where 70 per cent of all catalogued debris is found. Another debris field can be found farther out in geosynchro­nous orbit
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