HR1191 is a double main-sequence star in the constellation of Perseus.
HR1191 visual magnitude is 5.77. Because of its reltive faintness, HR1191 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 HR1191:
Celestial coordinates and finder chart of HR1191
HR1191 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 HR1191 are provided in the following table:
The simplified sky map below shows the position of HR1191 in the sky:
Visibility of HR1191 from your location
Digitized Sky Survey image of HR1191
The image below is a photograph of HR1191 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 HR1191 is 0.002 arcsec per year in Right Ascension and -0.007 arcsec per year in Declination and the associated displacement for the next 100000 years is represented with the red arrow.
Distance of HR1191 from the Sun and relative movement
HR1191 is distant 1,034.92 light years from the Sun and it is moving far from the Sun at the speed of 18 kilometers per second.
Spectral properties of HR1191
HR1191 belongs to spectral class B1 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR1191 is situated in the Hertzsprung–Russell diagram.
HR1191 star system properties
HR1191 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 HR1191 double sysyem: