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Long-term evolution of the space debris population Dr Hugh Lewis Astronautics Research Group, Faculty of Engineering & the Environment
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Space debris 101…
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Space debris sources
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Space debris population (1) Data courtesy of NASA Orbital Debris Program Office
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Space debris population (2) Softball size or larger ( 10 cm) ~22,000~500,000~100,000,000 Total mass: ~6,500 tonnes (> 2,700 tonnes in LEO) Marble size or larger ( 1 cm) Ball-point pen tip ( 1 mm)
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≥ 10 cm debris population ESA MASTER 2009 population seen in DAMAGE ~30,000 objects ≥ 10 cm May 2009
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View from the ISS Simulated view from the ISS, with orbiting objects from space-track ≥ 10 cm debris population
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UN space debris mitigation guidelines 1.Limit debris released during normal operations 2.Minimize the potential for break-ups during operational phases 3.Limit the probability of accidental collision in orbit 4.Avoid intentional destruction and other harmful activities 5.Minimize potential for post-mission break-ups resulting from stored energy 6.Limit the long-term presence of spacecraft and launch vehicle orbital stages in the low Earth orbit (LEO) region after the end of their mission 7.Limit the long-term interference of spacecraft and launch vehicle orbital stages with the geosynchronous (GEO) region after the end of their mission
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Remediation Even with good compliance with the commonly adopted mitigation guidelines, the space debris population is likely to grow: –Active Debris Removal About 50 removals needed to prevent one collision $1 – $3 billion per year
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LEO mitigation & remediation 30% compliance 90% compliance 90% compliance with 5 removals per year
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LEO mitigation & remediation 90% compliance 90% compliance with 5 removals per year Chance of the same result 1-in-501-in-2001-in-5
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12 Summary Compliance with debris mitigation guidelines is currently low –Even if compliance rates improve the debris population is likely to continue to grow: Catastrophic collisions every five to ten years Impact on spacecraft operations Remediation of the debris environment –Can help to limit the growth of the debris population: Activity needs to be sustained (expensive!) Catastrophic collisions will still occur Success is uncertain Challenges: –Compliance, Consensus, Cooperation, Collaboration, Contributions
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Thank you for your attention Contact: hglewis@soton.ac.uk Thanks to Holger Krag (ESA Space Debris Office) for permission to use the MASTER reference population, and J.-C. Liou (NASA Orbital Debris Program Office) for permission to use the satellite catalogue data
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