Occulter design for THEIA

N. Jeremy Kasdin; Eric J. Cady; Philip J. Dumont; P. Douglas Lisman; Stuart B. Shaklan; Remi Soummer; David N. Spergel; Robert J. Vanderbei

doi:10.1117/12.826518

19 August 2009 Occulter design for THEIA

N. Jeremy Kasdin, Eric J. Cady, Philip J. Dumont, P. Douglas Lisman, Stuart B. Shaklan, Remi Soummer, David N. Spergel, Robert J. Vanderbei

Author Affiliations +

Proceedings Volume 7440, Techniques and Instrumentation for Detection of Exoplanets IV; 744005 (2009) https://doi.org/10.1117/12.826518
Event: SPIE Optical Engineering + Applications, 2009, San Diego, California, United States

Abstract

An occulter is an instrument designed to suppress starlight by diffraction from its edges; most are designed to be circular, with a set of identical "petals" running around the outside. Proposed space-based occulters are lightweight, deployed screens tens of meters in diameter with challenging accuracy requirements. In this paper we describe the design of an occulter for the THEIA mission concept. THEIA consists of a 4-meter telescope diffraction limited to 300 nm, and a 40-meter external occulter to provide high-contrast imaging. Operating from 250 to 1000 nm, it will provide a rich family of science projects, including exoplanet characterization, ultraviolet spectroscopy, and very wide-field imaging. Originally conceived of as a hybrid system employing both an occulter and internal coronagraph, THEIA now uses a single occulter to achieve all of the starlight suppression but at two different distances from the telescope in order to minimize size and distance. We describe the basic design principles of the THEIA occulter, its final configuration, performance, and sensitivity.

Citation Download Citation

N. Jeremy Kasdin, Eric J. Cady, Philip J. Dumont, P. Douglas Lisman, Stuart B. Shaklan, Remi Soummer, David N. Spergel, and Robert J. Vanderbei "Occulter design for THEIA", Proc. SPIE 7440, Techniques and Instrumentation for Detection of Exoplanets IV, 744005 (19 August 2009); https://doi.org/10.1117/12.826518

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