Published October 20, 2004 | Version Published
Book Section - Chapter Open

Antarctic planet interferometer

  • 1. ROR icon Jet Propulsion Lab
  • 2. ROR icon University of Arizona
  • 3. ROR icon Harvard-Smithsonian Center for Astrophysics
  • 4. ROR icon UNSW Sydney
  • 5. ROR icon Paris Observatory
  • 6. ROR icon Université Côte d'Azur
  • 7. ROR icon California Institute of Technology
  • 8. ROR icon University of Sydney
  • 9. ROR icon Massachusetts Institute of Technology

Contributors

Abstract

The Antarctic Planet Interferometer is a concept for an instrument designed to detect and characterize extrasolar planets by exploiting the unique potential of the best accessible site on earth for thermal infrared interferometry. High-precision interferometric techniques under development for extrasolar planet detection and characterization (differential phase, nulling and astrometry) all benefit substantially from the slow, low-altitude turbulence, low water vapor content, and low temperature found on the Antarctic plateau. At the best of these locations, such as the Concordia base being developed at Dome C, an interferometer with two-meter diameter class apertures has the potential to deliver unique science for a variety of topics, including extrasolar planets, active galactic nuclei, young stellar objects, and protoplanetary disks.

Additional Information

© 2004 Society of Photo-optical Instrumentation Engineers (SPIE). The work described in this publication was carried out at the Jet Propulsion Laboratory, California Institute of Technology, under a contract with the National Aeronautics and Space Administration.

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Identifiers

Eprint ID
92280
Resolver ID
CaltechAUTHORS:20190115-105309152

Funding

NASA/JPL/Caltech

Dates

Created
2019-01-15
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Updated
2021-11-16
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Caltech Custom Metadata

Series Name
Proceedings of SPIE
Series Volume or Issue Number
5491