HR6317 is a main-sequence star in the constellation of Ophiuchus.
HR6317 visual magnitude is 6.59. Because of its reltive faintness, HR6317 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 HR6317:
Celestial coordinates and finder chart of HR6317
HR6317 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 HR6317 are provided in the following table:
The simplified sky map below shows the position of HR6317 in the sky:
Visibility of HR6317 from your location
Digitized Sky Survey image of HR6317
The image below is a photograph of HR6317 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 HR6317 is 0.044 arcsec per year in Right Ascension and -0.048 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR6317 from the Sun and relative movement
HR6317 is distant 238.13 light years from the Sun and it is moving towards the Sun at the speed of 10 kilometers per second.
Spectral properties of HR6317
HR6317 belongs to spectral class A7 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR6317 is situated in the Hertzsprung–Russell diagram.