HR7419 is a multiple giant star in the constellation of Cygnus.
HR7419 visual magnitude is 6.25. Because of its reltive faintness, HR7419 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 HR7419:
Celestial coordinates and finder chart of HR7419
HR7419 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 HR7419 are provided in the following table:
The simplified sky map below shows the position of HR7419 in the sky:
Visibility of HR7419 from your location
Digitized Sky Survey image of HR7419
The image below is a photograph of HR7419 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 HR7419 is 0.006 arcsec per year in Right Ascension and -0.011 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR7419 from the Sun and relative movement
HR7419 is distant 758.14 light years from the Sun and it is moving far from the Sun at the speed of 11 kilometers per second.
Spectral properties of HR7419
HR7419 belongs to spectral class B9 and has a luminosity class of III corresponding to a giant star.
The red dot in the diagram below shows where HR7419 is situated in the Hertzsprung–Russell diagram.
HR7419 star system properties
HR7419 is a visual double star which can be observed only with the help of very large telescopes. The table below shows key information about the HR7419 double sysyem: