An approach for the search of extra-solar system planets taking advantage of the simultaneous wide spectral range and high resolution of a future planetary observatory in earth orbit

Details An approach for the search of extra-solar system planets taking advantage of the simultaneous wide spectral range and high resolution of a future planetary observatory in earth orbit An approach for the search of extra-solar system planets taking advantage of the simultaneous wide spectral range and high resolution of a future planetary observatory in earth orbit

Nov 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992adspr..12..177b&link_type=abstract

(Planetary studies; Proceedings of Symposium 4 and the Topical Meeting of the Interdisciplinary Scientific Commission B /Meeting

Physics

2

Extrasolar Planets, Planetary Radiation, Spaceborne Telescopes, Stellar Spectra, Autocorrelation, Cross Correlation

Scientific paper

A new observational approach to the search for extra-solar planetary systems is presented which is based on high resolution spectroscopy, high coronographic efficiency, and long integration time. It is proposed to look for maxima in the cross-correlation function between the spectra of selected stars and their surrounding space. The Orbiting Planetary Telescope mission should be capable of meeting the following requirements: high rejection rate of the direct flux from the central star by coronographic techniques and the simultaneous access to a wide spectral range and a high spectral resolution.

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