HR7486 is a variable and double main-sequence star in the constellation of Aquila.
HR7486 visual magnitude is 6.01. Because of its reltive faintness, HR7486 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 HR7486:
Celestial coordinates and finder chart of HR7486
HR7486 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 HR7486 are provided in the following table:
The simplified sky map below shows the position of HR7486 in the sky:
Visibility of HR7486 from your location
Digitized Sky Survey image of HR7486
The image below is a photograph of HR7486 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 HR7486 is -0.002 arcsec per year in Right Ascension and -0.01 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR7486 from the Sun and relative movement
HR7486 is distant 1,646.46 light years from the Sun and it is moving towards the Sun at the speed of 14 kilometers per second.
Spectral properties of HR7486
HR7486 belongs to spectral class B5 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR7486 is situated in the Hertzsprung–Russell diagram.
HR7486 star system properties
HR7486 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 HR7486 double sysyem: