HR7275 is a variable sub-giant star in the constellation of Cygnus.
HR7275 visual magnitude is 5.81. Because of its reltive faintness, HR7275 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 HR7275:
Celestial coordinates and finder chart of HR7275
HR7275 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 HR7275 are provided in the following table:
The simplified sky map below shows the position of HR7275 in the sky:
Visibility of HR7275 from your location
HR7275 is circumpolar and transits at 18:39 UTC (altitude: 89.1°)
Digitized Sky Survey image of HR7275
The image below is a photograph of HR7275 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 HR7275 is -0.099 arcsec per year in Right Ascension and -0.059 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR7275 from the Sun and relative movement
HR7275 is distant 228.93 light years from the Sun and it is moving far from the Sun at the speed of 4 kilometers per second.
Spectral properties of HR7275
HR7275 belongs to spectral class K1 and has a luminosity class of IV corresponding to a sub-giant star.
The red dot in the diagram below shows where HR7275 is situated in the Hertzsprung–Russell diagram.