HR2679 is a main-sequence star in the constellation of Canis Major.
HR2679 visual magnitude is 6.48. Because of its reltive faintness, HR2679 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 HR2679:
Celestial coordinates and finder chart of HR2679
HR2679 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 HR2679 are provided in the following table:
The simplified sky map below shows the position of HR2679 in the sky:
Visibility of HR2679 from your location
Digitized Sky Survey image of HR2679
The image below is a photograph of HR2679 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 HR2679 is -0.018 arcsec per year in Right Ascension and 0.007 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR2679 from the Sun and relative movement
HR2679 is distant 4,939.39 light years from the Sun and it is moving far from the Sun at the speed of 33 kilometers per second.
Spectral properties of HR2679
HR2679 belongs to spectral class O7 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR2679 is situated in the Hertzsprung–Russell diagram.