HR1390 is a giant star in the constellation of Perseus.
HR1390 visual magnitude is 5.28. Because of its reltive faintness, HR1390 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 HR1390:
Celestial coordinates and finder chart of HR1390
HR1390 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 HR1390 are provided in the following table:
The simplified sky map below shows the position of HR1390 in the sky:
Visibility of HR1390 from your location
Digitized Sky Survey image of HR1390
The image below is a photograph of HR1390 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 HR1390 is 0.076 arcsec per year in Right Ascension and -0.11 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR1390 from the Sun and relative movement
HR1390 is distant 242.92 light years from the Sun and it is moving far from the Sun at the speed of 28 kilometers per second.
Spectral properties of HR1390
HR1390 belongs to spectral class K1 and has a luminosity class of III corresponding to a giant star.
The red dot in the diagram below shows where HR1390 is situated in the Hertzsprung–Russell diagram.