HR6776 is a double main-sequence star in the constellation of Ophiuchus.
HR6776 visual magnitude is 6.63. Because of its reltive faintness, HR6776 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 HR6776:
Celestial coordinates and finder chart of HR6776
HR6776 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 HR6776 are provided in the following table:
The simplified sky map below shows the position of HR6776 in the sky:
Visibility of HR6776 from your location
Digitized Sky Survey image of HR6776
The image below is a photograph of HR6776 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 HR6776 is 0.016 arcsec per year in Right Ascension and 0.008 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR6776 from the Sun and relative movement
HR6776 is distant 650.70 light years from the Sun and it is moving towards the Sun at the speed of 17 kilometers per second.
Spectral properties of HR6776
HR6776 belongs to spectral class A2 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR6776 is situated in the Hertzsprung–Russell diagram.
HR6776 star system properties
HR6776 is a visual double star which can be observed with binoculars or small telescopes. The table below shows key information about the HR6776 double sysyem: