HR7518 is a variable supergiant star in the constellation of Cygnus.
HR7518 visual magnitude is 6.82. Because of its reltive faintness, HR7518 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 HR7518:
Celestial coordinates and finder chart of HR7518
HR7518 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 HR7518 are provided in the following table:
The simplified sky map below shows the position of HR7518 in the sky:
Visibility of HR7518 from your location
Digitized Sky Survey image of HR7518
The image below is a photograph of HR7518 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 HR7518 is 0.001 arcsec per year in Right Ascension and -0.002 arcsec per year in Declination and the associated displacement for the next 100000 years is represented with the red arrow.
Distance of HR7518 from the Sun and relative movement
HR7518 is distant 6,392.16 light years from the Sun and it is moving towards the Sun at the speed of 36 kilometers per second.
Spectral properties of HR7518
HR7518 belongs to spectral class F2 and has a luminosity class of I corresponding to a supergiant star.
The red dot in the diagram below shows where HR7518 is situated in the Hertzsprung–Russell diagram.