Exoplanet detection from Dome C, Antarctica: opportunities and challenges

Abstract. Many methods have been proposed for the detection of exoplanets. The minimum detectable planetary size and mass, and the maximum distance from us at which exoplanets are observable, are determined by both technological and environmental constraints. The unique atmospheric conditions found...

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Bibliographic Details
Main Authors: C. Aime, F. Vakili, J. S. Lawrence, M. C. B. Ashley, M. G. Burton, J. W. V. Storey
Other Authors: The Pennsylvania State University CiteSeerX Archives
Format: Text
Language:English
Subjects:
telescopes
instrumentation
adaptive optics
atmospheric effects
techniques
Antarctic
Antarc*
Antarctica
Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.158.2964
http://www.phys.unsw.edu.au/~mcba/pubs/lawrence05.pdf
Description
Summary:Abstract. Many methods have been proposed for the detection of exoplanets. The minimum detectable planetary size and mass, and the maximum distance from us at which exoplanets are observable, are determined by both technological and environmental constraints. The unique atmospheric conditions found at Dome C offer significant advantages. Using what is now known about the turbulence profile of the atmosphere above Antarctic plateau sites, we explore the potential these sites offer for detecting exoplanets around nearby stars using various methods.

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