HR8788 is a main-sequence star in the constellation of Pegasus.
HR8788 visual magnitude is 6.13. Because of its reltive faintness, HR8788 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 HR8788:
Celestial coordinates and finder chart of HR8788
HR8788 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 HR8788 are provided in the following table:
The simplified sky map below shows the position of HR8788 in the sky:
Visibility of HR8788 from your location
Digitized Sky Survey image of HR8788
The image below is a photograph of HR8788 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 HR8788 is 0.232 arcsec per year in Right Ascension and 0.057 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR8788 from the Sun and relative movement
HR8788 is distant 140.76 light years from the Sun and it is moving towards the Sun at the speed of 12 kilometers per second.
Spectral properties of HR8788
HR8788 belongs to spectral class F6 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR8788 is situated in the Hertzsprung–Russell diagram.