12 October 2004 Extrasolar Planetary Imaging Coronagraph (EPIC)
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Abstract
The Extrasolar Planetary Imaging Coronagraph (EPIC) will provide the first direct measurements of a broad range of fundamental physical characteristics of giant planets in other solar systems. These characteristics include orbital inclination, mass, brightness, color, the presence (or absence) of CH4 and H2O, and orbital or rotational-driven variability. EPIC utilizes a 1.5 meter telescope coupled to a Visible Nulling Coronagraph to achieve these science goals. EPIC has been proposed as a Discovery Mission.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Mark Clampin, Gary J. Melnick, Richard G. Lyon, Holland Ford, J. Roger P. Angel, Daniel Y. Gezari, David A. Golimowski, George F. Hartig, Martin Harwit, Matt Holman, Garth D. Illingworth, Scott Kenyon, Douglas N.C. Lin, Mark Marley, Scot S. Olivier, Larry Petro, Dimitar D. Sasselov, Jean Louis Schneider, Sara Seager, Michael Shao, William Brian Sparks, Volker Tolls, Alycia Weinberger, Hsiao Smith, Ruth Chaing Carter, Robert A. Woodruff, Brent Hyatt, Stephen E. Kendrick, David Purmot, "Extrasolar Planetary Imaging Coronagraph (EPIC)", Proc. SPIE 5487, Optical, Infrared, and Millimeter Space Telescopes, (12 October 2004); doi: 10.1117/12.552314; https://doi.org/10.1117/12.552314
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KEYWORDS
Planets

Coronagraphy

Telescopes

Mirrors

Wavefronts

Stars

Space telescopes

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