HR8814 is a double sub-giant star in the constellation of Grus.
HR8814 visual magnitude is 5.81. Because of its reltive faintness, HR8814 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 HR8814:
Celestial coordinates and finder chart of HR8814
HR8814 is situated south of the celestial equator, as such, it is more easily visible from the southern emisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR8814 are provided in the following table:
The simplified sky map below shows the position of HR8814 in the sky:
Visibility of HR8814 from your location
HR8814 is currently not visible from Greenwich, United Kingdom [change]
Digitized Sky Survey image of HR8814
The image below is a photograph of HR8814 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 HR8814 is -0.325 arcsec per year in Right Ascension and -0.007 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR8814 from the Sun and relative movement
HR8814 is distant 112.92 light years from the Sun and it is moving far from the Sun at the speed of 12 kilometers per second.
Spectral properties of HR8814
HR8814 belongs to spectral class F4 and has a luminosity class of IV corresponding to a sub-giant star.
The red dot in the diagram below shows where HR8814 is situated in the Hertzsprung–Russell diagram.
HR8814 star system properties
HR8814 is a visual double star which can be observed with the help of large telescopes. The table below shows key information about the HR8814 double sysyem: