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Direct Imaging of Extra-Solar Planetary Systems with a Low-Scattered Light Telescope

  • R. J. Terrile
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 144)

Abstract

In a joint study conducted by the Jet Propulsion laboratory and the Perkin-Elmer Corporation it was found that an Earth orbital, one meter class low scattered light coronagraphic telescope can achieve a broad range of scientific objectives including the direct detection of Jupiter-sized planets around the nearby stars. Recent major advances in our understanding of coronagraphic performance and in the field of super smooth mirror fabrication allow such an instrument to be designed and built within current technology.

Keywords

Flux Ratio Diffract Light Primary Mirror Extrasolar Planet Nearby Star 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

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Copyright information

© Kluwer Academic Publishers 1988

Authors and Affiliations

  • R. J. Terrile
    • 1
  1. 1.Jet Propulsion Laboratory CalTechPasadenaUSA

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