The CORALIE survey for southern extrasolar planets: XVII. New and updated long period and massive planets

M Marmier, Damien Segransan, Stephane Dominique Udry, Michael Mayor, F Pepe, Didier Queloz, Christophe Lovis, Dominique Naef, Nuno C Santos, Roi Alonso, Susana Alves, S Berthet, Bruno Chazelas, Brice Olivier Demory, Xavier Dumusque, Anne Eggenberger, Pedro R L Figueira, Michael Gillon, Janis Hagelberg, M A LendlRosemary Anne Mardling, Denis Megevand, Marion Neveu, Johannes Sahlmann, Danuta Sosnowska, Malte Tewes, A H M J Triaud

Research output: Contribution to journalArticleResearchpeer-review

56 Citations (Scopus)


Context. Since 1998, a planet-search program around main sequence stars within 50 pc in the southern hemisphere has been carried out with the CORALIE echelle spectrograph at La Silla Observatory.

Aims. With an observing time span of more than 14 years, the CORALIE survey is now able to unveil Jovian planets on Jupiter's period domain. This growing period-interval coverage is important for building formation and migration models since observational constraints are still weak for periods beyond the ice line.

Methods. Long-term precise Doppler measurements with the CORALIE echelle spectrograph, together with a few additional observations made with the HARPS spectrograph on the ESO 3.6 m telescope, reveal radial velocity signatures of massive planetary companions on long-period orbits.

Results. In this paper we present seven new planets orbiting HD 27631, HD 98649, HD 106515A, HD 166724, HD 196067, HD 219077, and HD 220689, together with the CORALIE orbital parameters for three already known planets around HD 10647, HD 30562, and HD 86226. The period range of the new planetary companions goes from 2200 to 5500 days and covers a mass domain between 1 and 10.5 M-Jup. Surprisingly, five of them present very high eccentricities above e > 0 : 57. A pumping scenario by Kozai mechanism may be invoked for HD 106515Ab and HD 196067b, which are both orbiting stars in multiple systems. Since the presence of a third massive body cannot be inferred from the data of HD 98649b, HD 166724b, and HD 219077b, the origin of the eccentricity of these systems remains unknown. Except for HD 10647b, no constraint on the upper mass of the planets is provided by HIPPARCOS astrometric data. Finally, the hosts of these long period planets show no metallicity excess.
Original languageEnglish
Article numberA90
Number of pages13
JournalAstronomy & Astrophysics
Publication statusPublished - 2013

Cite this