Analytic Modeling of Starshades

Abstract

External occulters, otherwise known as starshades, have been proposed as a solution to one of the highest priority yet technically vexing problems facing astrophysics - the direct imaging and characterization of terrestrial planets around other stars. New apodization functions, developed over the past few years, now enable starshades of just a few tens of meters diameter to occult central stars so efficiently that the orbiting exoplanets can be revealed and other high contrast imaging challenges addressed. In this paper an analytic approach to analysis of these apodization functions is presented. It is used to develop a tolerance analysis suitable for use in designing practical starshades. The results provide a mathematical basis for understanding starshades and a quantitative approach to setting tolerances.

Astrophysical Journal, accepted for publication

References in corpus (3)

• Theoretical Limits on Extrasolar Terrestrial Planet Detection with Coronagraphs
• Optimal Occulter Design for Finding Extrasolar Planets
• The Big Occulting Steerable Satellite (BOSS)

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• Improvements on Fresnel arrays for high contrast imaging
• Optimization of starshades: focal plane versus pupil plane