HR8250 is a main-sequence star in the constellation of Pegasus.
HR8250 visual magnitude is 6.47. Because of its reltive faintness, HR8250 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 HR8250:
Celestial coordinates and finder chart of HR8250
HR8250 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 HR8250 are provided in the following table:
The simplified sky map below shows the position of HR8250 in the sky:
Visibility of HR8250 from your location
Digitized Sky Survey image of HR8250
The image below is a photograph of HR8250 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 HR8250 is 0.014 arcsec per year in Right Ascension and -0.041 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR8250 from the Sun and relative movement
HR8250 is distant 225.61 light years from the Sun and it is moving far from the Sun at the speed of 14 kilometers per second.
Spectral properties of HR8250
HR8250 belongs to spectral class F7 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR8250 is situated in the Hertzsprung–Russell diagram.