Abstract
One of the main candidates for creating high-contrast for future Exo-Earth detection is an external occulter or sharshade. A starshade blocks the light from the parent star by flying in formation along the line-of-sight from a space telescope. Because of its large size and scale it is impossible to fully test a starshade system on the ground before launch. Instead, we rely on modeling supported by subscale laboratory tests to verify the models. At Princeton, we are designing and building a subscale testbed to verify the suppression and contrast of a starshade at the same Fresnel number as a flight system, and thus mathematically identical to a realistic space mission. Here we present the mechanical design of the testbed and simulations predicting the ultimate contrast performance. We will also present progress in implementation and preliminary results.
Original language | English |
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Title of host publication | Techniques and Instrumentation for Detection of Exoplanets VII |
Editors | Stuart Shaklan |
Publisher | SPIE |
ISBN (Electronic) | 9781628417715 |
DOIs | |
Publication status | Published - 2015 |
Event | Techniques and Instrumentation for Detection of Exoplanets VII - San Diego, United States Duration: 2015 Aug 10 → 2015 Aug 13 |
Publication series
Name | Proceedings of SPIE - The International Society for Optical Engineering |
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Volume | 9605 |
ISSN (Print) | 0277-786X |
ISSN (Electronic) | 1996-756X |
Other
Other | Techniques and Instrumentation for Detection of Exoplanets VII |
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Country/Territory | United States |
City | San Diego |
Period | 15/8/10 → 15/8/13 |
Bibliographical note
Publisher Copyright:© 2015 SPIE.
All Science Journal Classification (ASJC) codes
- Electronic, Optical and Magnetic Materials
- Condensed Matter Physics
- Computer Science Applications
- Applied Mathematics
- Electrical and Electronic Engineering