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Published on: September 20, 2017
Multiple-Star System Adaptive Vortex Coronagraphy Using a Liquid Crystal Light Valve.
Artur Aleksanyan1, Nina Kravets1, Etienne Brasselet1
1Université Bordeaux, CNRS, LOMA, UMR 5798, F-33400 Talence, France.
We developed a new imaging technique to block multiple light sources simultaneously. This allows for the direct observation of exoplanets orbiting multiple stars.
Area of Science:
- * Astronomy and astrophysics
- * Optical engineering
- * Exoplanet detection
Background:
- * Directly observing exoplanets is challenging due to the overwhelming glare of their host stars.
- * Current coronagraphy techniques are often limited in their ability to suppress multiple bright sources simultaneously.
- * The search for Earth-like planets in complex stellar systems requires advanced imaging capabilities.
Purpose of the Study:
- * To develop a novel high-contrast imaging technique for simultaneous suppression of multiple light sources.
- * To demonstrate a reconfigurable multiple-vortex phase mask for adaptive optical nulling.
- * To enable the direct observation and characterization of exoplanets in multi-star systems.
Main Methods:
- * Development of a reconfigurable multiple-vortex phase mask using a liquid crystal thin film.
- * Electro-optical addressing of local topological features on the phase mask.
- * Laboratory demonstration of triple-star optical vortex coronagraphy.
Main Results:
- * Successful simultaneous nulling of three light sources was achieved in a laboratory setting.
- * The technique utilizes a reconfigurable liquid crystal phase mask with addressable topological features.
- * The method is scalable to higher multiplicities of light sources.
Conclusions:
- * The proposed technique offers a significant advancement in high-contrast imaging for astronomical observations.
- * This technology facilitates the direct observation and analysis of complex extrasolar planetary systems, including those with multiple suns.
- * Future applications include the study of potentially habitable exoplanets in binary and multiple-star configurations.

