HR7550 is a double main-sequence star in the constellation of Cygnus.
HR7550 visual magnitude is 6.53. Because of its reltive faintness, HR7550 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 HR7550:
Celestial coordinates and finder chart of HR7550
HR7550 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 HR7550 are provided in the following table:
The simplified sky map below shows the position of HR7550 in the sky:
Visibility of HR7550 from your location
Digitized Sky Survey image of HR7550
The image below is a photograph of HR7550 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 HR7550 is 0.085 arcsec per year in Right Ascension and 0.062 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR7550 from the Sun and relative movement
HR7550 is distant 217.48 light years from the Sun and it is moving towards the Sun at the speed of 27 kilometers per second.
Spectral properties of HR7550
HR7550 belongs to spectral class F4 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR7550 is situated in the Hertzsprung–Russell diagram.
HR7550 star system properties
HR7550 is a visual double star which can be observed with the help of large telescopes. The table below shows key information about the HR7550 double sysyem: