Volume 447, Number 1, February III 2006
|Page(s)||397 - 403|
|Published online||27 January 2006|
Fundamental limitations on Earth-like planet detection with extremely large telescopes
LESIA, Observatoire de Paris Meudon, 5 Pl. J. Janssen, 92195 Meudon, France e-mail: firstname.lastname@example.org
2 ONERA, BP 52, 29 avenue de la Division Leclerc, 92320 Châtillon Cedex, France
Accepted: 20 September 2005
We analyse the fundamental limitations for the detection of extraterrestrial planets with Extremely Large Telescopes. For this task, a coronagraphic device combined with a very high order wavefront correction system is required but is not sufficient to achieve the 10-10 contrast level needed to detect an Earth-like planet. The stellar residuals left uncorrected by the wavefront correction system need to be calibrated and subtracted. We consider a general model including the dynamic phase aberrations downstream of the wavefront correction system, the static phase aberrations of the instrument and some differential aberrations provided by the calibration unit. A rather optimistic case of a filled circular pupil and of a perfect coronagraph is assumed. As a result of the analytical study, the limitation is found to mostly come from the static aberrations. We confirm this result using numerical simulations and evaluate the requirements in terms of phase aberrations to detect Earth-like planets with Extremely Large Telescopes.
Key words: techniques: high angular resolution / instrumentation: adaptive optics / stars: imaging / stars: planetary systems
© ESO, 2006
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.