HR6427 is a double main-sequence star in the constellation of Scorpius.
HR6427 visual magnitude is 6.65. Because of its reltive faintness, HR6427 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 HR6427:
Celestial coordinates and finder chart of HR6427
HR6427 is situated south of the celestial equator, as such, it is more easily visible from the southern emisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR6427 are provided in the following table:
The simplified sky map below shows the position of HR6427 in the sky:
Visibility of HR6427 from your location
HR6427 is currently not visible from Greenwich, United Kingdom [change]
Digitized Sky Survey image of HR6427
The image below is a photograph of HR6427 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 HR6427 is -0.007 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 HR6427 from the Sun and relative movement
HR6427 is distant 928.77 light years from the Sun and it is moving towards the Sun at the speed of 15 kilometers per second.
Spectral properties of HR6427
HR6427 belongs to spectral class B9 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR6427 is situated in the Hertzsprung–Russell diagram.
HR6427 star system properties
HR6427 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 HR6427 double sysyem: