EDP Sciences
Free access
Volume 445, Number 3, January III 2006
Page(s) 1143 - 1149
Section Planets and planetary systems
DOI http://dx.doi.org/10.1051/0004-6361:20042384

A&A 445, 1143-1149 (2006)
DOI: 10.1051/0004-6361:20042384

Ground-based direct detection of close-in extra-solar planets with nulling and high order adaptive optics

M. Langlois1, A. Burrows2 and P. Hinz2

1  Laboratoire d'Astophysique de Marseille, 2 place Le Verrier, 13248 Marseille, France
    e-mail: maud.langlois@oamp.fr
2  Steward Observatory, Tucson, AZ 85719, USA

(Received 17 November 2004 / Accepted 11 April 2005)

Ground-based direct detection of extra-solar planets is very challenging due to high planet to star brightness contrasts. For giant close-in planets, such as have been discovered by the radial velocity method, closer than 0.1 AU, the reflected light is predicted to be fairly high yielding a contrast ratio ranging from 10-4 to 10-5 at near infra-red wavelengths. In this paper, we investigate direct detection of reflected light from such planets using nulling interferometry, and high-order adaptive optics in conjunction with large double aperture ground-based telescopes. In this configuration, at least 10-3 suppression of the entire stellar Airy pattern with small loss of planet flux as close as 0.03 arcsec is achievable. Distinguishing residual starlight from the planet signal is achieved by using the center of gravity shift method or multicolor differential imaging. Using these assumptions, we derive exposure times from a few minutes to several hours for direct detection of many of the known extra-solar planets with several short-baseline double aperture telescopes such as the Large Binocular Telescope (LBT), the Very Large Telescope (VLT) and the Keck Telescope.

Key words: stars: planetary systems -- instrumentation: interferometers -- instrumentation: high angular resolution -- instrumentation: adaptive optics

SIMBAD Objects

© ESO 2006