HR7569 is a variable and double hypergiant star in the constellation of Aquila.
HR7569 visual magnitude is 6.13. Because of its reltive faintness, HR7569 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 HR7569:
Celestial coordinates and finder chart of HR7569
HR7569 is situated close to the celestial equator, as such, it is at least partly visible from both hemispheres in certain times of the year. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR7569 are provided in the following table:
The simplified sky map below shows the position of HR7569 in the sky:
Visibility of HR7569 from your location
Digitized Sky Survey image of HR7569
The image below is a photograph of HR7569 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 HR7569 is -0.335 arcsec per year in Right Ascension and -0.32 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR7569 from the Sun and relative movement
HR7569 is distant 90.18 light years from the Sun and it is moving towards the Sun at the speed of 17 kilometers per second.
Spectral properties of HR7569
HR7569 belongs to spectral class G0 and has a luminosity class of V corresponding to a hypergiant star.
The red dot in the diagram below shows where HR7569 is situated in the Hertzsprung–Russell diagram.
HR7569 star system properties
HR7569 is a visual double star which can be observed with the help of small or medium telescopes. The table below shows key information about the HR7569 double sysyem: