HR5325 is a main-sequence star in the constellation of Centaurus.
HR5325 visual magnitude is 6.31. Because of its reltive faintness, HR5325 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 HR5325:
Celestial coordinates and finder chart of HR5325
HR5325 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 HR5325 are provided in the following table:
The simplified sky map below shows the position of HR5325 in the sky:
Visibility of HR5325 from your location
HR5325 is currently not visible from Greenwich, United Kingdom [change]
Digitized Sky Survey image of HR5325
The image below is a photograph of HR5325 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 HR5325 is 0.137 arcsec per year in Right Ascension and -0.142 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR5325 from the Sun and relative movement
HR5325 is distant 68.62 light years from the Sun and it is moving far from the Sun at the speed of 3 kilometers per second.
Spectral properties of HR5325
HR5325 belongs to spectral class F9 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR5325 is situated in the Hertzsprung–Russell diagram.