Laboratory demonstrations of high-contrast imaging for space coronagraphy
2007
Space coronagraphy is a promising method for direct imaging of planetary systems orbiting the nearby stars. The High
Contrast Imaging Testbed is a laboratory facility at JPL that integrates the essential hardware and control algorithms
needed for suppression of diffracted and scattered light near a target star that would otherwise obscure an associated
exo-planetary system. Stable suppression of starlight by a factor of 5×10 −10 has been demonstrated consistently in
narrowband light over fields of view as close as four Airy radii from the star. Recent progress includes the extension of
spectral bandwidths to 10% at contrast levels of 2×10 −9 , with work in progress to further improve contrast levels,
bandwidth, and instrument throughput. We summarize recent laboratory results and outline future directions. This
laboratory experience is used to refine computational models, leading to performance and tolerance predictions for
future space mission architectures.
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