HR6843 is a main-sequence star in the constellation of Serpens.
HR6843 visual magnitude is 6.31. Because of its reltive faintness, HR6843 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 HR6843:
Celestial coordinates and finder chart of HR6843
HR6843 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 HR6843 are provided in the following table:
The simplified sky map below shows the position of HR6843 in the sky:
Visibility of HR6843 from your location
Digitized Sky Survey image of HR6843
The image below is a photograph of HR6843 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 HR6843 is 0.009 arcsec per year in Right Ascension and -0.056 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR6843 from the Sun and relative movement
HR6843 is distant 430.08 light years from the Sun and it is moving towards the Sun at the speed of 14 kilometers per second.
Spectral properties of HR6843
HR6843 belongs to spectral class A8 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR6843 is situated in the Hertzsprung–Russell diagram.