HR6496 is a main-sequence star in the constellation of Serpens.
HR6496 visual magnitude is 6.21. Because of its reltive faintness, HR6496 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 HR6496:
Celestial coordinates and finder chart of HR6496
HR6496 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 HR6496 are provided in the following table:
The simplified sky map below shows the position of HR6496 in the sky:
Visibility of HR6496 from your location
Digitized Sky Survey image of HR6496
The image below is a photograph of HR6496 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 HR6496 is 0.037 arcsec per year in Right Ascension and -0.062 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR6496 from the Sun and relative movement
HR6496 is distant 147.64 light years from the Sun and it is moving towards the Sun at the speed of 40 kilometers per second.
Spectral properties of HR6496
HR6496 belongs to spectral class F7 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR6496 is situated in the Hertzsprung–Russell diagram.