HR2450 is a bright giant star in the constellation of Canis Major.
HR2450 visual magnitude is 4.82. Because of its moderate brightness, HR2450 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 HR2450:
Celestial coordinates and finder chart of HR2450
HR2450 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 HR2450 are provided in the following table:
The simplified sky map below shows the position of HR2450 in the sky:
Visibility of HR2450 from your location
Digitized Sky Survey image of HR2450
The image below is a photograph of HR2450 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 HR2450 is 0.004 arcsec per year in Right Ascension and -0.004 arcsec per year in Declination and the associated displacement for the next 100000 years is represented with the red arrow.
Distance of HR2450 from the Sun and relative movement
HR2450 is distant 1,574.88 light years from the Sun and it is moving far from the Sun at the speed of 29 kilometers per second.
Spectral properties of HR2450
HR2450 belongs to spectral class K2 and has a luminosity class of II corresponding to a bright giant star.
The red dot in the diagram below shows where HR2450 is situated in the Hertzsprung–Russell diagram.