HR1424 is a double main-sequence star in the constellation of Perseus.
HR1424 visual magnitude is 6.26. Because of its reltive faintness, HR1424 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 HR1424:
Celestial coordinates and finder chart of HR1424
HR1424 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 HR1424 are provided in the following table:
The simplified sky map below shows the position of HR1424 in the sky:
Visibility of HR1424 from your location
HR1424 is circumpolar and transits at 04:37 UTC (altitude: 78.5°)
Digitized Sky Survey image of HR1424
The image below is a photograph of HR1424 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 HR1424 is -0.006 arcsec per year in Right Ascension and -0.014 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR1424 from the Sun and relative movement
HR1424 is distant 1,706.81 light years from the Sun and it is moving towards the Sun at the speed of 12 kilometers per second.
Spectral properties of HR1424
HR1424 belongs to spectral class B8 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR1424 is situated in the Hertzsprung–Russell diagram.
HR1424 star system properties
HR1424 is a visual double star which can be observed with the help of small or medium telescopes. The table below shows key information about the HR1424 double sysyem: