HR6873 is a variable main-sequence star in the constellation of Serpens.
HR6873 visual magnitude is 6.13. Because of its reltive faintness, HR6873 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 HR6873:
Celestial coordinates and finder chart of HR6873
HR6873 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 HR6873 are provided in the following table:
The simplified sky map below shows the position of HR6873 in the sky:
Visibility of HR6873 from your location
Digitized Sky Survey image of HR6873
The image below is a photograph of HR6873 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 HR6873 is 0.013 arcsec per year in Right Ascension and -0.004 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR6873 from the Sun and relative movement
HR6873 is distant 3,360.82 light years from the Sun and it is moving towards the Sun at the speed of 18 kilometers per second.
Spectral properties of HR6873
HR6873 belongs to spectral class B3 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR6873 is situated in the Hertzsprung–Russell diagram.