HR8899 is a main-sequence star in the constellation of Pegasus.
HR8899 visual magnitude is 6.69. Because of its reltive faintness, HR8899 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 HR8899:
Celestial coordinates and finder chart of HR8899
HR8899 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 HR8899 are provided in the following table:
The simplified sky map below shows the position of HR8899 in the sky:
Visibility of HR8899 from your location
Digitized Sky Survey image of HR8899
The image below is a photograph of HR8899 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 HR8899 is 0.232 arcsec per year in Right Ascension and 0.04 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR8899 from the Sun and relative movement
HR8899 is distant 234.36 light years from the Sun and it is moving far from the Sun at the speed of 10 kilometers per second.
Spectral properties of HR8899
HR8899 belongs to spectral class F4 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR8899 is situated in the Hertzsprung–Russell diagram.