HR6412 is a variable main-sequence star in the constellation of Ophiuchus.
HR6412 visual magnitude is 6.17. Because of its reltive faintness, HR6412 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 HR6412:
Celestial coordinates and finder chart of HR6412
HR6412 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 HR6412 are provided in the following table:
The simplified sky map below shows the position of HR6412 in the sky:
Visibility of HR6412 from your location
Digitized Sky Survey image of HR6412
The image below is a photograph of HR6412 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 HR6412 is 0.001 arcsec per year in Right Ascension and -0.021 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR6412 from the Sun and relative movement
HR6412 is distant 588.45 light years from the Sun and it is moving far from the Sun at the speed of 4 kilometers per second.
Spectral properties of HR6412
HR6412 belongs to spectral class A2 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR6412 is situated in the Hertzsprung–Russell diagram.