HR466 is a double main-sequence star in the constellation of Cetus.
HR466 visual magnitude is 6.24. Because of its reltive faintness, HR466 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 HR466:
Celestial coordinates and finder chart of HR466
HR466 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 HR466 are provided in the following table:
The simplified sky map below shows the position of HR466 in the sky:
Visibility of HR466 from your location
Digitized Sky Survey image of HR466
The image below is a photograph of HR466 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 HR466 is 0.259 arcsec per year in Right Ascension and 0.093 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR466 from the Sun and relative movement
HR466 is distant 124.67 light years from the Sun and it is moving far from the Sun at the speed of 48 kilometers per second.
Spectral properties of HR466
HR466 belongs to spectral class F7 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR466 is situated in the Hertzsprung–Russell diagram.
HR466 star system properties
HR466 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 HR466 double sysyem: