HR7484 is a variable main-sequence star in the constellation of Cygnus.
HR7484 visual magnitude is 5.82. Because of its reltive faintness, HR7484 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 HR7484:
Celestial coordinates and finder chart of HR7484
HR7484 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 HR7484 are provided in the following table:
The simplified sky map below shows the position of HR7484 in the sky:
Visibility of HR7484 from your location
HR7484 is circumpolar and transits at 11:04 UTC (altitude: 86.5°)
Digitized Sky Survey image of HR7484
The image below is a photograph of HR7484 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 HR7484 is 0.035 arcsec per year in Right Ascension and 0.164 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR7484 from the Sun and relative movement
HR7484 is distant 129.78 light years from the Sun and it is moving towards the Sun at the speed of 15 kilometers per second.
Spectral properties of HR7484
HR7484 belongs to spectral class F6 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR7484 is situated in the Hertzsprung–Russell diagram.