HR325 is a main-sequence star in the constellation of Cetus.
HR325 visual magnitude is 6.37. Because of its reltive faintness, HR325 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 HR325:
Celestial coordinates and finder chart of HR325
HR325 is situated close to the celestial equator, as such, it is at least partly visible from both hemispheres in certain times of the year. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR325 are provided in the following table:
The simplified sky map below shows the position of HR325 in the sky:
Visibility of HR325 from your location
Digitized Sky Survey image of HR325
The image below is a photograph of HR325 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 HR325 is 0.098 arcsec per year in Right Ascension and -0.036 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR325 from the Sun and relative movement
HR325 is distant 233.52 light years from the Sun and it is moving far from the Sun at the speed of 15 kilometers per second.
Spectral properties of HR325
HR325 belongs to spectral class A7 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR325 is situated in the Hertzsprung–Russell diagram.