High Angular Resolution and Extrasolar Planets: Beyond Basic Instrumental Performances

Details High Angular Resolution and Extrasolar Planets: Beyond Basic Instrumental Performances High Angular Resolution and Extrasolar Planets: Beyond Basic Instrumental Performances

May 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001sf2a.conf..489s&link_type=abstract

Abstracts from SF2A-2001: Semaine de l'Astrophysique Francaise, meeting held in Lyon, France, May 28-June 1st, 2001, Eds.: F. Co

Astronomy and Astrophysics

Astrophysics

Scientific paper

I will review: 1. The characteristics of planetary systems for which high angular resolution is required. 2. The implications for the specifications of "optical architectures" (angular resolution, spectral range and resolution, dynamics etc). I will emphasize the "thresholds" above which new perspectives are open (e.g. from giant to Earth-like planets). 3. The different architectures proposed for Darwin, TPF and their possible precursors.

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