HR1324 is a variable main-sequence star in the constellation of Perseus.
HR1324 visual magnitude is 4.61. Because of its moderate brightness, HR1324 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 HR1324:
Celestial coordinates and finder chart of HR1324
HR1324 is situated north of the celestial equator, as such, it is more easily visible from the northern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR1324 are provided in the following table:
The simplified sky map below shows the position of HR1324 in the sky:
Visibility of HR1324 from your location
HR1324 is circumpolar and transits at 04:24 UTC (altitude: 88.8°)
Digitized Sky Survey image of HR1324
The image below is a photograph of HR1324 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 HR1324 is 0.047 arcsec per year in Right Ascension and -0.054 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR1324 from the Sun and relative movement
HR1324 is distant 318.05 light years from the Sun and it is moving far from the Sun at the speed of 20 kilometers per second.
Spectral properties of HR1324
HR1324 belongs to spectral class A2 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR1324 is situated in the Hertzsprung–Russell diagram.