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09/18/14 SO/NOAO Joint Colloquium Series: Andrew Skemer

Room: 

Andrew Skemer, Steward Observatory

Imaging Exoplanets with the LBT

Abstract:

By directly imaging extrasolar planets, we can study the compositions, atmospheric properties and interiors of gas-giant planets, and eventually, the surfaces of rocky planets. The current generation of directly imaged planets are abnormally warm, and future exoplanet studies will target cooler, "normal" planets, which emit the majority of their light in the mid-infrared (>3 microns). At these wavelengths, the Large Binocular Telescope is unique in its capabilities as a high-contrast exoplanet imager. I will describe a multi-faceted program at the LBT to study planets in the mid-infrared where we are (1) executing a large survey to search for new exoplanets, using instrumentation that is sensitive to lower-mass and smaller separation exoplanets than were visible to previous surveys, (2) studying the properties of the small number of massive, widely-separated exoplanets that are currently accessible to direct imaging, and (3) developing new optics and instrumentation to improve our ability to discover and characterize exoplanets.

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