HR1455 is a double bright giant star in the constellation of Taurus.
HR1455 visual magnitude is 6.36. Because of its reltive faintness, HR1455 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 HR1455:
Celestial coordinates and finder chart of HR1455
HR1455 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 HR1455 are provided in the following table:
The simplified sky map below shows the position of HR1455 in the sky:
Visibility of HR1455 from your location
Digitized Sky Survey image of HR1455
The image below is a photograph of HR1455 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 HR1455 is -0.001 arcsec per year in Right Ascension and -0.017 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR1455 from the Sun and relative movement
HR1455 is distant 463.73 light years from the Sun and it is moving towards the Sun at the speed of 2 kilometers per second.
Spectral properties of HR1455
HR1455 belongs to spectral class G5 and has a luminosity class of II corresponding to a bright giant star.
The red dot in the diagram below shows where HR1455 is situated in the Hertzsprung–Russell diagram.
HR1455 star system properties
HR1455 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 HR1455 double sysyem: