2009/12/31 by N. C. Santos, M. Mayor, W. Benz +11 · 2 citations
Physics and Astronomy · #Astro and Planetary Science #Astrobiology #Astronomy #Astrophysics #Astrophysics and Star Formation Studies #Physics #Planet #Stars #Stellar, planetary, and galactic studies #astro-ph.EP #astro-ph.SR
paper · pdf · doi:10.1051/0004-6361/200913489
Accepted for publication in A&A (replaced by version with minor language corrections)
openalex publication_date 2010/01/15 · arxiv created 2010/01/28 · arxiv updated 2015/05/14 · openalex created_date 2016/06/24 · openalex updated_date 2026/08/05
We present the discovery of three new giant planets around three metal-deficient stars: HD 5388 b (1.96 <i>M<i/><sub>Jup<sub/>), HD 181720 b (0.37 <i>M<i/><sub>Jup<sub/>), and HD 190984 b (3.1 <i>M<i/><sub>Jup<sub/>). All the planets have moderately eccentric orbits (ranging from 0.26 to 0.57) and long orbital periods (from 777 to 4885 days). Two of the stars (HD 181720 and HD 190984) were part of a program searching for giant planets around a sample of ~100 moderately metal-poor stars, while HD 5388 was part of the volume-limited sample of the HARPS GTO program. Our discoveries suggest that giant planets in long period orbits are not uncommon around moderately metal-poor stars.