 Mission system’s engineer, Marie-Claire Perkinson, at EADS Astrium UK, describes how their proposal was a response to a Planetary Society competition.
‘The approach we took was to have a very stable orbit around the asteroid,’ says Perkinson. ‘Sending a radio signal to a spacecraft and returning it could measure very accurately the distance to the spacecraft and enable us to reconstruct the orbit of the asteroid's center of mass. If we do that over a long period, we could determine very accurately the orbit of the asteroid itself.’
She continues, ‘one of the things we'd be looking at is wide and narrow angle, low and high-resolution mapping of the surface of the asteroid. From that you can also determine the shape of the asteroid.’
The most novel aspect of EADS Astrium’s approach is the thermal measurement of the Yarkovsky Effect. This phenomenon occurs as the asteroid rotates. The heat from the sun on one side of the asteroid is released back into space. Temperature variation across the surface affects the orbital path.
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