HR4767 is a main-sequence star in the constellation of Ursa Major.
HR4767 visual magnitude is 6.21. Because of its reltive faintness, HR4767 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 HR4767:
Celestial coordinates and finder chart of HR4767
HR4767 is situated north of the celestial equator, as such, it is more easily visible from the northern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR4767 are provided in the following table:
The simplified sky map below shows the position of HR4767 in the sky:
Visibility of HR4767 from your location
HR4767 is circumpolar and transits at 12:31 UTC (altitude: 88.4°)
Digitized Sky Survey image of HR4767
The image below is a photograph of HR4767 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 HR4767 is 0.015 arcsec per year in Right Ascension and 0.181 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR4767 from the Sun and relative movement
HR4767 is distant 71.52 light years from the Sun and it is moving towards the Sun at the speed of 21 kilometers per second.
Spectral properties of HR4767
HR4767 belongs to spectral class F8 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR4767 is situated in the Hertzsprung–Russell diagram.