Extrasolar planet characteristics in the visible wavelength range

Details Extrasolar planet characteristics in the visible wavelength range Extrasolar planet characteristics in the visible wavelength range

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003esasp.539..231t&link_type=abstract

In: Proceedings of the Conference on Towards Other Earths: DARWIN/TPF and the Search for Extrasolar Terrestrial Planets, 22-25 A

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Extrasolar Planets, Visible Wavelengths, Color, Color-Color Diagram, Spectra, Coronagraphs

Scientific paper

A coronagraph operating in the visible wavelength range to detect and characterize extrasolar planets offers advantages over any other wavelength range. The physical characteristics of a planet and its atmosphere can be derived from its color and its low-resolution spectrum, both of which are discussed. An analytic method is presented for calculating the shapes of mirrors in a pupil-mapping coronagraph.

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