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 50 light-years away from the Sun in the constellation of Ara.

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, 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 constellation. Based on the spectral type (G5V), Cervantes colour is yellow, a mid-ranged temperature star.

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 in the constellation and is easily visible to the naked eye under dark skies.

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 visible to the naked eye only from locations with very dark skies, while it is not visible at all from skies affected by light pollution.

Oct 10, 2024 · mu Ara c is a Confirmed extrasolar planet (exoplanet) that orbits the star Cervantes in the constellation of Ara

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 star approximately 50 light-years away from the Sun in the constellation of Ara.

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 lists all planets in the system mu Arae. This table lists all stars in the system mu Arae.

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.

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.