HR756 is a main-sequence star in the constellation of Andromeda.
HR756 visual magnitude is 5.9. Because of its reltive faintness, HR756 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 HR756:
Celestial coordinates and finder chart of HR756
HR756 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 HR756 are provided in the following table:
The simplified sky map below shows the position of HR756 in the sky:
Visibility of HR756 from your location
HR756 is circumpolar and transits at 22:02 UTC (altitude: 77.3°)
Digitized Sky Survey image of HR756
The image below is a photograph of HR756 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 HR756 is 0.145 arcsec per year in Right Ascension and -0.194 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR756 from the Sun and relative movement
HR756 is distant 176.98 light years from the Sun and it is moving far from the Sun at the speed of 1 kilometers per second.
Spectral properties of HR756
HR756 belongs to spectral class F5 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR756 is situated in the Hertzsprung–Russell diagram.