Lockheed Martin engineers have designed and built a prototype nine-aperture wide-field imaging telescope that overcomes the increase in mass, volume and cost associated with large single-optics telescopes for space-based applications. The ability of a telescope to resolve fine detail is a direct function of its light-gathering power. Larger apertures -- mirrors or lenses -- gather more light and provide greater resolution of detail.
"The key to making a distributed aperture optical system work is to properly phase the individual modules. Phasing means that all telescopes present an equal path length, to tolerances considerably less than the wavelength of light," said Star-9 program manager Peter Dean. "We have demonstrated the fundamental feasibility of this approach with the Star-9 test bed and quantified performance with subsequent test bed activities."
The prototype, called Star-9 due to the number and arrangement of apertures, uses multiple small telescope modules that yield a system with a much larger effective aperture. This distributed aperture imaging approach provides a new path to affordable high resolution by packaging the modules in a smaller envelope thus reducing the size, weight, and cost of the system.
Multiple apertures also provide a multifunctional capability unavailable with a single monolithic mirror. A distributed-aperture approach could be incorporated in space-based remote sensing instruments that might use individual telescope modules, or groups of modules, to simultaneously view a scene at several different wavelengths or polarizations. On subsequent orbits the system could be reconfigured.
Adaptability and flexibility is a key feature since several small apertures can be grouped as a sub-array to image multiple objects on a single pass.
Distributed aperture imaging technology also provides redundancy, reliability, and lower risk. A single failure in a monolithic mirror system could ruin a mission, while the loss of a single aperture in a multiple aperture system could be overcome.
The performance demonstrations used off-the-shelf focal planes, electronics and mirror actuators. The experiments show clearly that high-quality imagery can be acquired over a useful field of view for an Earth-imaging or an astronomical-distributed-aperture imaging system.
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