Ground-Based Interferometry

Details Ground-Based Interferometry Ground-Based Interferometry

Mar 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996ap%26ss.241..105s&link_type=abstract

Astrophysics and Space Science, Volume 241, Issue 1, pp.105-110

Astronomy and Astrophysics

Astrophysics

2

Scientific paper

This paper summarizes the limits of ground-based interferometry for differential astrometry as well as ground-based interferometry for direct detection of exo-planets and exo-zodi dust levels. For direct detection, ground-based interferometry at near IR wavelengths using large telescopes with adaptive optics offers a significant advantage over single telescopes with adaptive optics. Ground-based differential astrometry for exo-planet detection is extremely accurate with sufficient accuracy to detect Neptune mass planets around 400 600 nearby stars. Ground-based interferometry using large (>6m) telescopes is also capable of detecting the 10 μm emission of the zodiacal light around nearby stars with zodi levels similar to our solar system

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