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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

  • eBook Packages: Springer Book Archive

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