HR5485 is a giant star in the constellation of Centaurus.
HR5485 visual magnitude is 4.05. Because of its moderate brightness, HR5485 should be easily visible from locations with dark skyes, while it can be barely visible, or not visible at all, from skyes affected by light pollution.
The table below summarizes the key facts about HR5485:
Celestial coordinates and finder chart of HR5485
HR5485 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 HR5485 are provided in the following table:
The simplified sky map below shows the position of HR5485 in the sky:
Visibility of HR5485 from your location
Digitized Sky Survey image of HR5485
The image below is a photograph of HR5485 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 HR5485 is -0.064 arcsec per year in Right Ascension and -0.18 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR5485 from the Sun and relative movement
HR5485 is distant 205.16 light years from the Sun and it is moving towards the Sun at the speed of 38 kilometers per second.
Spectral properties of HR5485
HR5485 belongs to spectral class K3 and has a luminosity class of III corresponding to a giant star.
The red dot in the diagram below shows where HR5485 is situated in the Hertzsprung–Russell diagram.