HR7508 is a variable and double main-sequence star in the constellation of Vulpecula.
HR7508 visual magnitude is 6.28. Because of its reltive faintness, HR7508 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 HR7508:
Celestial coordinates and finder chart of HR7508
HR7508 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 HR7508 are provided in the following table:
The simplified sky map below shows the position of HR7508 in the sky:
Visibility of HR7508 from your location
Digitized Sky Survey image of HR7508
The image below is a photograph of HR7508 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 HR7508 is -0.009 arcsec per year in Right Ascension and 0.004 arcsec per year in Declination and the associated displacement for the next 100000 years is represented with the red arrow.
Distance of HR7508 from the Sun and relative movement
HR7508 is distant 4,346.67 light years from the Sun and it is moving towards the Sun at the speed of 12 kilometers per second.
Spectral properties of HR7508
HR7508 belongs to spectral class B7 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR7508 is situated in the Hertzsprung–Russell diagram.
HR7508 star system properties
HR7508 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 HR7508 double sysyem: