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Title: High resolution telescope including an array of elemental telescopes aligned along a common axis and supported on a space frame with a pivot at its geometric center

Patent ·
OSTI ID:868258

A large effective-aperture, low-cost optical telescope with diffraction-limited resolution enables ground-based observation of near-earth space objects. The telescope has a non-redundant, thinned-aperture array in a center-mount, single-structure space frame. It employes speckle interferometric imaging to achieve diffraction-limited resolution. The signal-to-noise ratio problem is mitigated by moving the wavelength of operation to the near-IR, and the image is sensed by a Silicon CCD. The steerable, single-structure array presents a constant pupil. The center-mount, radar-like mount enables low-earth orbit space objects to be tracked as well as increases stiffness of the space frame. In the preferred embodiment, the array has elemental telescopes with subaperture of 2.1 m in a circle-of-nine configuration. The telescope array has an effective aperture of 12 m which provides a diffraction-limited resolution of 0.02 arc seconds. Pathlength matching of the telescope array is maintained by a electro-optical system employing laser metrology. Speckle imaging relaxes pathlength matching tolerance by one order of magnitude as compared to phased arrays. Many features of the telescope contribute to substantial reduction in costs. These include eliminating the conventional protective dome and reducing on-site construction activities. The cost of the telescope scales with the first power of the aperture rather than its third power as in conventional telescopes.

Research Organization:
Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States)
DOE Contract Number:
W-7405-ENG-48
Assignee:
United States of America as represented by United States (Washington, DC)
Patent Number(s):
US 5108168
OSTI ID:
868258
Country of Publication:
United States
Language:
English

References (8)

Aperture Synthesis Using Independent Telescopes journal January 1970
Point Arrays Having Compact, Nonredundant Autocorrelations journal January 1971
Performance Characteristics Of Phased Array And Thinned Aperture Optical Telescopes journal September 1988
Interferometric imaging in optical astronomy journal November 1988
Noise considerations in stellar speckle interferometry*† journal January 1977
Multiple mirror telescope as a phased array telescope journal January 1985
Design Considerations For Multiple Telescope Imaging Arrays journal September 1988
Low-cost, high-resolution telescopes for imaging low-earth-orbit satellites conference July 1990

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