HR5085 is a multiple main-sequence star in the constellation of Ursa Major.
HR5085 visual magnitude is 5.4. Because of its reltive faintness, HR5085 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 HR5085:
Celestial coordinates and finder chart of HR5085
HR5085 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 HR5085 are provided in the following table:
The simplified sky map below shows the position of HR5085 in the sky:
Visibility of HR5085 from your location
HR5085 is circumpolar and transits at 08:59 UTC (altitude: 81.5°)
Digitized Sky Survey image of HR5085
The image below is a photograph of HR5085 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 HR5085 is -0.08 arcsec per year in Right Ascension and 0.037 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR5085 from the Sun and relative movement
HR5085 is distant 236.40 light years from the Sun and it is moving towards the Sun at the speed of 3 kilometers per second.
Spectral properties of HR5085
HR5085 belongs to spectral class A1 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR5085 is situated in the Hertzsprung–Russell diagram.
HR5085 star system properties
HR5085 is a visual double star which can be observed with binoculars or small telescopes. The table below shows key information about the HR5085 double sysyem: