HR483 is a main-sequence star in the constellation of Andromeda.
HR483 visual magnitude is 4.95. Because of its moderate brightness, HR483 should be easily visible from locations with dark skyes, while it can be barely visible, or not visible at all, from skyes affected by light pollution.
The table below summarizes the key facts about HR483:
Celestial coordinates and finder chart of HR483
HR483 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 HR483 are provided in the following table:
The simplified sky map below shows the position of HR483 in the sky:
Visibility of HR483 from your location
HR483 is circumpolar and transits at 20:56 UTC (altitude: 81.1°)
Digitized Sky Survey image of HR483
The image below is a photograph of HR483 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 HR483 is 0.809 arcsec per year in Right Ascension and -0.154 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR483 from the Sun and relative movement
HR483 is distant 41.22 light years from the Sun and it is moving far from the Sun at the speed of 4 kilometers per second.
Spectral properties of HR483
HR483 belongs to spectral class G1 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR483 is situated in the Hertzsprung–Russell diagram.