HR5629

HR5629 is a main-sequence star in the constellation of Ursa Minor.

HR5629 visual magnitude is 6.13. Because of its reltive faintness, HR5629 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 HR5629:

Celestial coordinates and finder chart of HR5629

HR5629 is situated close to the northern celestial pole and, as such, it is visible for most part of the year from the northern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR5629 are provided in the following table:

The simplified sky map below shows the position of HR5629 in the sky:

Visibility of HR5629 from your location

HR5629 is circumpolar and transits at 22:15 UTC (altitude: 75.6°)

Digitized Sky Survey image of HR5629

The image below is a photograph of HR5629 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 HR5629 is 0.023 arcsec per year in Right Ascension and -0.007 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.

Distance of HR5629 from the Sun and relative movement

HR5629 is distant 463.73 light years from the Sun and it is moving towards the Sun at the speed of 5 kilometers per second.

Spectral properties of HR5629

HR5629 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 HR5629 is situated in the Hertzsprung–Russell diagram.

Alternative designations of HR5629