HR1074 is a variable main-sequence star in the constellation of Perseus.
HR1074 visual magnitude is 5.9. Because of its reltive faintness, HR1074 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 HR1074:
Celestial coordinates and finder chart of HR1074
HR1074 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 HR1074 are provided in the following table:
The simplified sky map below shows the position of HR1074 in the sky:
Visibility of HR1074 from your location
Digitized Sky Survey image of HR1074
The image below is a photograph of HR1074 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 HR1074 is -0.01 arcsec per year in Right Ascension and 0.001 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR1074 from the Sun and relative movement
HR1074 is distant 1,638.19 light years from the Sun and it is moving far from the Sun at the speed of 25 kilometers per second.
Spectral properties of HR1074
HR1074 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 HR1074 is situated in the Hertzsprung–Russell diagram.