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Proceedings Article

Adaptive nulling: a new enabling technology for interferometric exo-planet detection

[+] Author Affiliations
Oliver P. Lay, Muthu Jeganathan, Robert Peters

Jet Propulsion Lab. (USA)

Proc. SPIE 5170, Techniques and Instrumentation for Detection of Exoplanets, 103 (November 21, 2003); doi:10.1117/12.503759
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From Conference Volume 5170

  • Techniques and Instrumentation for Detection of Exoplanets
  • Daniel R. Coulter
  • San Diego, California, USA | August 03, 2003

abstract

Deep, stable nulling of starlight requires careful control of the amplitudes and phases of the beams that are being combined. The detection of earth-like planets using the interferometer architectures currently being considered for the Terrestrial Planet Finder mission require that the E-field amplitudes are balanced at the level of ~ 0.1%, and the phases are controlled at the level of 1 mrad (corresponding to ~ 1.5 nm for a wavelength of 10 μm). These conditions must be met simultaneously at all wavelengths across the science band, and for both polarization states, imposing unrealistic tolerances on the symmetry between the optical beamtrains. We introduce the concept of a compensator that is inserted into the beamtrain, which can adaptively correct for the mismatches across the spectrum, enabling deep nulls with realistic, imperfect optics. The design presented uses a deformable mirror to adjust the amplitude and phase of each beam as an arbitrary function of wavelength and polarization. A proof-of-concept experiment will be conducted at visible / near-IR wavelengths, followed by a system operating in the Mid-IR band.

© (2003) COPYRIGHT SPIE--The International Society for Optical Engineering. Downloading of the abstract is permitted for personal use only.
Citation

Oliver P. Lay ; Muthu Jeganathan and Robert Peters
"Adaptive nulling: a new enabling technology for interferometric exo-planet detection", Proc. SPIE 5170, Techniques and Instrumentation for Detection of Exoplanets, 103 (November 21, 2003); doi:10.1117/12.503759; http://dx.doi.org/10.1117/12.503759


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