HR6613 is a double main-sequence star in the constellation of Scorpius.
HR6613 visual magnitude is 6.43. Because of its reltive faintness, HR6613 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 HR6613:
Celestial coordinates and finder chart of HR6613
HR6613 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 HR6613 are provided in the following table:
The simplified sky map below shows the position of HR6613 in the sky:
Visibility of HR6613 from your location
Digitized Sky Survey image of HR6613
The image below is a photograph of HR6613 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 HR6613 is -0.002 arcsec per year in Right Ascension and -0.007 arcsec per year in Declination and the associated displacement for the next 100000 years is represented with the red arrow.
Distance of HR6613 from the Sun and relative movement
HR6613 is distant 381.29 light years from the Sun and it is moving far from the Sun at the speed of 1 kilometers per second.
Spectral properties of HR6613
HR6613 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 HR6613 is situated in the Hertzsprung–Russell diagram.
HR6613 star system properties
HR6613 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 HR6613 double sysyem: