HR8765 is a sub-giant star in the constellation of Pegasus.
HR8765 visual magnitude is 6.57. Because of its reltive faintness, HR8765 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 HR8765:
Celestial coordinates and finder chart of HR8765
HR8765 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 HR8765 are provided in the following table:
The simplified sky map below shows the position of HR8765 in the sky:
Visibility of HR8765 from your location
Digitized Sky Survey image of HR8765
The image below is a photograph of HR8765 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 HR8765 is 0.005 arcsec per year in Right Ascension and -0.016 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR8765 from the Sun and relative movement
HR8765 is distant 381.73 light years from the Sun and it is moving towards the Sun at the speed of 17 kilometers per second.
Spectral properties of HR8765
HR8765 belongs to spectral class F2 and has a luminosity class of IV corresponding to a sub-giant star.
The red dot in the diagram below shows where HR8765 is situated in the Hertzsprung–Russell diagram.