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Proceedings Paper

Planetscope: an exoplanet coronagraph on a balloon platform
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Paper Abstract

Direct detection of mature exoplanets is possible using a visible-wavelength telescope and coronagraph in the stratosphere. We analyze two sources of dynamic wavefront perturbations: turbulence in the free atmosphere and locally generated turbulence. We find that they are expected to have relatively small effects on the wavefront. We find that neither source should limit observations at 10-9 contrast levels for planet-star separations of 0.5 arcsec. On this basis, we expect that it is feasible to image and characterize several known radial-velocity exoplanets.

Paper Details

Date Published: 14 July 2008
PDF: 12 pages
Proc. SPIE 7010, Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter, 70103S (14 July 2008); doi: 10.1117/12.788087
Show Author Affiliations
Wesley A. Traub, Jet Propulsion Lab. (United States)
Pin Chen, Jet Propulsion Lab. (United States)
Brian Kern, Jet Propulsion Lab. (United States)
Taro Matsuo, Jet Propulsion Lab. (United States)
Japanese Society for the Promotion of Science (Japan)

Published in SPIE Proceedings Vol. 7010:
Space Telescopes and Instrumentation 2008: Optical, Infrared, and Millimeter
Jacobus M. Oschmann Jr.; Mattheus W. M. de Graauw; Howard A. MacEwen, Editor(s)

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