Mu Arae (μ Arae, abbreviated Mu Ara, μ Ara), often designated HD 160691, officially named Cervantes / sɜːrˈvæntiːz / sur-VAN-teez, [8] is a main sequence G-type star approximately 50 …

Oct 24, 2024 · HD 160691 b is a gas giant exoplanet that orbits a G-type star. Its mass is 4.3 Jupiters, it takes 1.8 years to complete one orbit of its star, and is 1.5 AU from its star. Its …

Spectroscopic [Fe/H] for 98 extra-solar planet-host stars. Exploring the probability of planet formation. Statistical properties of exoplanets. II. Metallicity, orbital parameters, and space …

Mu Arae c, also known as HD 160691 c, formally named Dulcinea (pronounced / d ʌ l ˈ s ɪ n i ə / or / d ʌ l s ɪ ˈ n iː ə /), [3] is an extrasolar planet orbiting the star Mu Arae of the constellation Ara.

Mar 28, 2003 · We show that the currently available Doppler data rather preclude the 2:1 mean motion resonance expected by some authors to be present in the HD 160691 planetary system.

Apr 1, 2005 · We perform a dynamical analysis of the recently updated set of the radial velocity (RV) measurements of HD 160691 (μ Arae). The kinematic, double-Keplerian model of the …

Oct 24, 2024 · HD 160691 c is a gas giant exoplanet that orbits a G-type star. Its mass is 4.4 Jupiters, it takes 10.8 years to complete one orbit of its star, and is 4.17 AU from its star. Its …

Jun 13, 2002 · We also report further observations of the metal rich planet bearing star HD 160691. Our new solution confirms the previously reported planet and shows a trend indicating …

Jan 27, 2003 · The orbits in the HD 160691 planetary system at first appeared highly unstable, but using the MEGNO and FLI techniques of global dynamics analysis in the orbital parameter …

Mu Arae b, often designated HD 160691 b and formally named Quijote / kiˈhoʊtiː /, is an exoplanet orbiting the star Mu Arae in the constellation Ara. The planet has at least one and a …