HR1141 is a double main-sequence star in the constellation of Perseus.
HR1141 visual magnitude is 5.66. Because of its reltive faintness, HR1141 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 HR1141:
Celestial coordinates and finder chart of HR1141
HR1141 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 HR1141 are provided in the following table:
The simplified sky map below shows the position of HR1141 in the sky:
Visibility of HR1141 from your location
HR1141 is circumpolar and transits at 03:51 UTC (altitude: 84.2°)
Digitized Sky Survey image of HR1141
The image below is a photograph of HR1141 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 HR1141 is 0.023 arcsec per year in Right Ascension and -0.018 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR1141 from the Sun and relative movement
HR1141 is distant 1,038.22 light years from the Sun and it is moving far from the Sun at the speed of 2 kilometers per second.
Spectral properties of HR1141
HR1141 belongs to spectral class B6 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR1141 is situated in the Hertzsprung–Russell diagram.
HR1141 star system properties
HR1141 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 HR1141 double sysyem: