HR1589 is a double main-sequence star in the constellation of Camelopardalis.
HR1589 visual magnitude is 5.96. Because of its reltive faintness, HR1589 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 HR1589:
Celestial coordinates and finder chart of HR1589
HR1589 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 HR1589 are provided in the following table:
The simplified sky map below shows the position of HR1589 in the sky:
Visibility of HR1589 from your location
HR1589 is circumpolar and transits at 00:18 UTC (altitude: 67.4°)
Digitized Sky Survey image of HR1589
The image below is a photograph of HR1589 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 HR1589 is 0.013 arcsec per year in Right Ascension and -0.016 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR1589 from the Sun and relative movement
HR1589 is distant 537.07 light years from the Sun and it is moving towards the Sun at the speed of 9 kilometers per second.
Spectral properties of HR1589
HR1589 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 HR1589 is situated in the Hertzsprung–Russell diagram.
HR1589 star system properties
HR1589 is a visual double star which can be observed with the help of large telescopes. The table below shows key information about the HR1589 double sysyem: