HR1289 is a main-sequence star in the constellation of Cepheus.
HR1289 visual magnitude is 5.57. Because of its reltive faintness, HR1289 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 HR1289:
Celestial coordinates and finder chart of HR1289
HR1289 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 HR1289 are provided in the following table:
The simplified sky map below shows the position of HR1289 in the sky:
Visibility of HR1289 from your location
HR1289 is circumpolar and transits at 03:44 UTC (altitude: 57.7°)
Digitized Sky Survey image of HR1289
The image below is a photograph of HR1289 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 HR1289 is -0.014 arcsec per year in Right Ascension and 0.01 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR1289 from the Sun and relative movement
HR1289 is distant 684.87 light years from the Sun and it is moving towards the Sun at the speed of 7 kilometers per second.
Spectral properties of HR1289
HR1289 belongs to spectral class B5 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR1289 is situated in the Hertzsprung–Russell diagram.