HR5189 is a double sub-giant star in the constellation of Centaurus.
HR5189 visual magnitude is 6.53. Because of its reltive faintness, HR5189 should be visible only from locations with dark skyes, while it is not visible at all from skyes affected by light pollution.
The table below summarizes the key facts about HR5189:
Celestial coordinates and finder chart of HR5189
HR5189 is situated south of the celestial equator, as such, it is more easily visible from the southern emisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR5189 are provided in the following table:
The simplified sky map below shows the position of HR5189 in the sky:
Visibility of HR5189 from your location
Digitized Sky Survey image of HR5189
The image below is a photograph of HR5189 from the Digitized Sky Survey 2 (DSS2 - see the credits section) taken in the red channel. The area of sky represented in the image is 0.5x0.5 degrees (30x30 arcmins). The proper motion of HR5189 is -0.516 arcsec per year in Right Ascension and -0.174 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR5189 from the Sun and relative movement
HR5189 is distant 92.22 light years from the Sun and it is moving far from the Sun at the speed of 4 kilometers per second.
Spectral properties of HR5189
HR5189 belongs to spectral class G3 and has a luminosity class of IV corresponding to a sub-giant star.
The red dot in the diagram below shows where HR5189 is situated in the Hertzsprung–Russell diagram.
HR5189 star system properties
HR5189 is a visual double star which can be observed with the help of small or medium telescopes. The table below shows key information about the HR5189 double sysyem: