HR8292 is a sub-giant star in the constellation of Pegasus.
HR8292 visual magnitude is 6.09. Because of its reltive faintness, HR8292 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 HR8292:
Celestial coordinates and finder chart of HR8292
HR8292 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 HR8292 are provided in the following table:
The simplified sky map below shows the position of HR8292 in the sky:
Visibility of HR8292 from your location
Digitized Sky Survey image of HR8292
The image below is a photograph of HR8292 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 HR8292 is 0.024 arcsec per year in Right Ascension and -0.002 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR8292 from the Sun and relative movement
HR8292 is distant 696.58 light years from the Sun and it is moving far from the Sun at the speed of 6 kilometers per second.
Spectral properties of HR8292
HR8292 belongs to spectral class B5 and has a luminosity class of IV corresponding to a sub-giant star.
The red dot in the diagram below shows where HR8292 is situated in the Hertzsprung–Russell diagram.