Abstract
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 tnterferometry 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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© 1996 Springer Science+Business Media New York
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Shao, M. (1996). Ground-Based Interferometry. In: Shull, J.M., Thronson, H.A., Stern, S.A. (eds) The Search for Extra-Solar Terrestrial Planets: Techniques and Technology. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5808-4_9
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DOI: https://doi.org/10.1007/978-94-011-5808-4_9
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-6453-8
Online ISBN: 978-94-011-5808-4
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