HR8397 is a variable giant star in the constellation of Pegasus.
HR8397 visual magnitude is 6.37. Because of its reltive faintness, HR8397 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 HR8397:
Celestial coordinates and finder chart of HR8397
HR8397 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 HR8397 are provided in the following table:
The simplified sky map below shows the position of HR8397 in the sky:
Visibility of HR8397 from your location
Digitized Sky Survey image of HR8397
The image below is a photograph of HR8397 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 HR8397 is 0.022 arcsec per year in Right Ascension and 0.003 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR8397 from the Sun and relative movement
HR8397 is distant 1,341.56 light years from the Sun and it is moving towards the Sun at the speed of 15 kilometers per second.
Spectral properties of HR8397
HR8397 belongs to spectral class B5 and has a luminosity class of III corresponding to a giant star.
The red dot in the diagram below shows where HR8397 is situated in the Hertzsprung–Russell diagram.