25 September 2012 Adaptive optics for laser space debris removal
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Space debris in low Earth orbit below 1500km is becoming an increasing threat to satellites and spacecrafts. Radar and laser tracking are currently used to monitor the orbits of thousands of space debris and active satellites are able to use this information to manoeuvre out of the way of a predicted collision. However, many satellites are not able to manoeuvre and debris-on debris collisions are becoming a signicant contributor to the growing space debris population. The removal of the space debris from orbit is the preferred and more definitive solution. Space debris removal may be achieved through laser ablation, whereby a high power laser corrected with an adaptive optics system could, in theory, allow ablation of the debris surface and so impart a remote thrust on the targeted object. The goal of this is to avoid collisions between space debris to prevent an exponential increase in the number of space debris objects. We are developing an experiment to demonstrate the feasibility of laser ablation for space debris removal. This laser ablation demonstrator utilises a pulsed sodium laser to probe the atmosphere ahead of the space debris and the sun reflection of the space debris is used to provide atmospheric tip{tilt information. A deformable mirror is then shaped to correct an infrared laser beam on the uplink path to the debris. We present here the design and the expected performance of the system.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Francis Bennet, Francis Bennet, Rodolphe Conan, Rodolphe Conan, Celine D'Orgeville, Celine D'Orgeville, Murray Dawson, Murray Dawson, Nicolas Paulin, Nicolas Paulin, Ian Price, Ian Price, Francois Rigaut, Francois Rigaut, Ian Ritchie, Ian Ritchie, Craig Smith, Craig Smith, Kristina Uhlendorf, Kristina Uhlendorf, } "Adaptive optics for laser space debris removal", Proc. SPIE 8447, Adaptive Optics Systems III, 844744 (25 September 2012); doi: 10.1117/12.925773; https://doi.org/10.1117/12.925773


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