HR391 is a multiple main-sequence star in the constellation of Cassiopeia.
HR391 visual magnitude is 6.45. Because of its reltive faintness, HR391 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 HR391:
Celestial coordinates and finder chart of HR391
HR391 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 HR391 are provided in the following table:
The simplified sky map below shows the position of HR391 in the sky:
Visibility of HR391 from your location
HR391 is circumpolar and transits at 16:13 UTC (altitude: 83.3°)
Digitized Sky Survey image of HR391
The image below is a photograph of HR391 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 HR391 is 0.139 arcsec per year in Right Ascension and -0.094 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR391 from the Sun and relative movement
HR391 is distant 188.00 light years from the Sun and it is moving far from the Sun at the speed of 7 kilometers per second.
Spectral properties of HR391
HR391 belongs to spectral class F4 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR391 is situated in the Hertzsprung–Russell diagram.
HR391 star system properties
HR391 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 HR391 double sysyem: