HR6919 is a variable main-sequence star in the constellation of Sagittarius.
HR6919 visual magnitude is 6.2. Because of its reltive faintness, HR6919 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 HR6919:
Celestial coordinates and finder chart of HR6919
HR6919 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 HR6919 are provided in the following table:
The simplified sky map below shows the position of HR6919 in the sky:
Visibility of HR6919 from your location
Digitized Sky Survey image of HR6919
The image below is a photograph of HR6919 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 HR6919 is -0.004 arcsec per year in Right Ascension and 0.007 arcsec per year in Declination and the associated displacement for the next 100000 years is represented with the red arrow.
Distance of HR6919 from the Sun and relative movement
HR6919 is distant 566.96 light years from the Sun and it is moving towards the Sun at the speed of 35 kilometers per second.
Spectral properties of HR6919
HR6919 belongs to spectral class B8 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR6919 is situated in the Hertzsprung–Russell diagram.