Please use this identifier to cite or link to this item: http://hdl.handle.net/10773/15055
Title: Detectability of quasi-circular co-orbital planets: application to the radial velocity technique
Author: Leleu, Adrien
Robutel, Philippe
Correia, Alexandre C. M.
Keywords: Planets and satellites - detection
Planets and satellites - dynamical evolution and stability
Celestial mechanics
Issue Date: 22-Sep-2015
Publisher: EDP Sciences, ESO
Abstract: Several celestial bodies in co-orbital configurations exist in the solar system. However, co-orbital exoplanets have not yet been discovered. This lack may result from a degeneracy between the signal induced by co-orbital planets and other orbital configurations. Here we determine a criterion for the detectability of quasi-circular co-orbital planets and develop a demodulation method to bring out their signature from the observational data. We show that the precision required to identify a pair of co-orbital planets depends only on the libration amplitude and on the planet's mass ratio. We apply our method to synthetic radial velocity data, and show that for tadpole orbits we are able to determine the inclination of the system to the line of sight. Our method is also valid for planets detected through the transit and astrometry techniques.
Peer review: yes
URI: http://hdl.handle.net/10773/15055
DOI: 10.1051/0004-6361/201526175
ISSN: 1432-0746
Appears in Collections:CIDMA - Artigos
DFis - Artigos
GGDG - Artigos

Files in This Item:
File Description SizeFormat 
Leleu_etal_2015.pdf1.68 MBAdobe PDFView/Open


FacebookTwitterDeliciousLinkedInDiggGoogle BookmarksMySpace
Formato BibTex MendeleyEndnote Degois 

Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.