HR611 is a supergiant star in the constellation of Cetus.
HR611 visual magnitude is 5.62. Because of its reltive faintness, HR611 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 HR611:
Celestial coordinates and finder chart of HR611
HR611 is situated close to the celestial equator, as such, it is at least partly visible from both hemispheres in certain times of the year. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR611 are provided in the following table:
The simplified sky map below shows the position of HR611 in the sky:
Visibility of HR611 from your location
Digitized Sky Survey image of HR611
The image below is a photograph of HR611 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 HR611 is 0.006 arcsec per year in Right Ascension and -0.068 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR611 from the Sun and relative movement
HR611 is distant 654.62 light years from the Sun and it is moving far from the Sun at the speed of 25 kilometers per second.
Spectral properties of HR611
HR611 belongs to spectral class K5 and has a luminosity class of I corresponding to a supergiant star.
The red dot in the diagram below shows where HR611 is situated in the Hertzsprung–Russell diagram.