
Mu Arae - Wikipedia
Mu Arae (μ Arae, abbreviated Mu Ara, μ Ara), often designated HD 160691, officially named Cervantes / s ɜːr ˈ v æ n t iː z / sur-VAN-teez, [8] is a main sequence G-type star approximately …
Mu Arae c - Wikipedia
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.
Cervantes Star Facts (Mu Arae) - Universe Guide
Cervantes, also known as Mu Arae is a main sequence star located in the constellation of Ara, The Altar. It is not part of the Ara constellation outline but is within the borders of the …
Mu Arae - Space Wiki
Mu Arae (μ Arae, abbreviated Mu Ara, μ Ara) is a yellow main-sequence star located in the constellation Ara, approximately 50 light-years (15 parsecs) from Earth. It is the brightest star …
Cervantes - μ Arae (mu Arae) - Star in Ara | TheSkyLive.com
Cervantes, also designated as μ Arae (mu Arae), is a sub-giant star of spectral class G3 in the constellation of Ara. Cervantes visual magnitude is 5.15. Because of its faintness, Cervantes is …
Mu Ara C Exoplanet Facts - Universe Guide
Oct 10, 2024 · mu Ara c is a Confirmed extrasolar planet (exoplanet) that orbits the star Cervantes in the constellation of Ara
Mu Arae - Wikiwand
Mu Arae c, the innermost, was the first hot Neptune or super-Earth discovered. Mu Arae, often designated HD 160691, officially named Cervantes sur-VAN-teez, is a main sequence G-type …
Open Exoplanet Catalogue - mu Arae c
The planetary system mu Arae hosts at least 4 planets. This list shows all planetary and stellar components in the system. It gives a quick overview of the hierarchical architecture. This table …
Exoplanet Mu Arae d | Stellar Catalog
Exoplanet Mu Arae d orbits star Mu Arae that lies 51 light years away from the Sun. It weighs about 165.9 Earth masses and orbits its star closer than Earth orbits Sun.
Mu Arae - Stellar Catalog
Subgiant Mu Arae is located 51 light years away from the Sun. It is a single star of spectral class G3IV-V C, that has 110 % of solar mass. There are multiple known exoplanets in this system.
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