HR5547 is a bright giant star in the constellation of Apus.
HR5547 visual magnitude is 5.93. Because of its reltive faintness, HR5547 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 HR5547:
Celestial coordinates and finder chart of HR5547
HR5547 is situated close to the southern celestial pole and, as such, it is easilty visible for most part of the year from the southern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR5547 are provided in the following table:
The simplified sky map below shows the position of HR5547 in the sky:
Visibility of HR5547 from your location
Digitized Sky Survey image of HR5547
The image below is a photograph of HR5547 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 HR5547 is -0.003 arcsec per year in Right Ascension and 0.004 arcsec per year in Declination and the associated displacement for the next 100000 years is represented with the red arrow.
Distance of HR5547 from the Sun and relative movement
HR5547 is distant 876.34 light years from the Sun and it is moving far from the Sun at the speed of 2 kilometers per second.
Spectral properties of HR5547
HR5547 belongs to spectral class G8 and has a luminosity class of II corresponding to a bright giant star.
The red dot in the diagram below shows where HR5547 is situated in the Hertzsprung–Russell diagram.