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Adaptive Optics for Direct Detection of Extrasolar Planets: The Gemini Planet Imager

Journal Article · · Comptes rendus - Physique, vol. 8, no. 3-4, April 1, 2007, pp. 365-373
The direct detection of photons emitted or reflected by extrasolar planets, spatially resolved from their parent star, is a major frontier in the study of other solar systems. Direct detection will provide statistical information on planets in 5-50 AU orbits, inaccessible to current Doppler searches, and allow spectral characterization of radius, temperature, surface gravity, and perhaps composition. Achieving this will require new dedicated high-contrast instruments. One such system under construction is the Gemini Planet Imager (GPI.) This combines a high-order/high-speed adaptive optics system to control wavefront errors from the Earth's atmosphere, an advanced coronagraph to block diffraction, ultrasmooth optics, a precision infrared interferometer to measure and correct systematic errors, and a integral field spectrograph/polarimeter to image and characterize target planetary systems. We predict that GPI will be able to detect planets with brightness less than 10{sup -7} of their parent star, sufficient to observe warm self-luminous planets around a large population of targets.
Research Organization:
Lawrence Livermore National Laboratory (LLNL), Livermore, CA
Sponsoring Organization:
USDOE
DOE Contract Number:
W-7405-ENG-48
OSTI ID:
950621
Report Number(s):
UCRL-JRNL-230274
Journal Information:
Comptes rendus - Physique, vol. 8, no. 3-4, April 1, 2007, pp. 365-373, Journal Name: Comptes rendus - Physique, vol. 8, no. 3-4, April 1, 2007, pp. 365-373 Journal Issue: 3-4 Vol. 8
Country of Publication:
United States
Language:
English

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