HR1234 is a hypergiant star in the constellation of Perseus.
HR1234 visual magnitude is 6.41. Because of its reltive faintness, HR1234 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 HR1234:
Celestial coordinates and finder chart of HR1234
HR1234 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 HR1234 are provided in the following table:
The simplified sky map below shows the position of HR1234 in the sky:
Visibility of HR1234 from your location
Digitized Sky Survey image of HR1234
The image below is a photograph of HR1234 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 HR1234 is -0.022 arcsec per year in Right Ascension and 0.015 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR1234 from the Sun and relative movement
HR1234 is distant 373.00 light years from the Sun and it is moving towards the Sun at the speed of 20 kilometers per second.
Spectral properties of HR1234
HR1234 belongs to spectral class A0 and has a luminosity class of V corresponding to a hypergiant star.
The red dot in the diagram below shows where HR1234 is situated in the Hertzsprung–Russell diagram.