HR7412 is a variable and multiple supergiant star in the constellation of Aquila.
HR7412 visual magnitude is 6.09. Because of its reltive faintness, HR7412 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 HR7412:
Celestial coordinates and finder chart of HR7412
HR7412 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 HR7412 are provided in the following table:
The simplified sky map below shows the position of HR7412 in the sky:
Visibility of HR7412 from your location
Digitized Sky Survey image of HR7412
The image below is a photograph of HR7412 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 HR7412 is -0.005 arcsec per year in Right Ascension and 0 arcsec per year in Declination and the associated displacement for the next 100000 years is represented with the red arrow.
Distance of HR7412 from the Sun and relative movement
HR7412 is distant 1,663.27 light years from the Sun and it is moving towards the Sun at the speed of 13 kilometers per second.
Spectral properties of HR7412
HR7412 belongs to spectral class K5 and has a luminosity class of I corresponding to a supergiant star.
The red dot in the diagram below shows where HR7412 is situated in the Hertzsprung–Russell diagram.
HR7412 star system properties
HR7412 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 HR7412 double sysyem: