HR6578 is a variable supergiant star in the constellation of Ophiuchus.
HR6578 visual magnitude is 6.19. Because of its reltive faintness, HR6578 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 HR6578:
Celestial coordinates and finder chart of HR6578
HR6578 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 HR6578 are provided in the following table:
The simplified sky map below shows the position of HR6578 in the sky:
Visibility of HR6578 from your location
Today's HR6578 rise, transit and set times from Greenwich, United Kingdom are the following (all times relative to the local timezone Europe/London):
Digitized Sky Survey image of HR6578
The image below is a photograph of HR6578 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 HR6578 is -0.023 arcsec per year in Right Ascension and -0.018 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR6578 from the Sun and relative movement
HR6578 is distant 544.24 light years from the Sun and it is moving towards the Sun at the speed of 49 kilometers per second.
Spectral properties of HR6578
HR6578 belongs to spectral class K2 and has a luminosity class of I corresponding to a supergiant star.
The red dot in the diagram below shows where HR6578 is situated in the Hertzsprung–Russell diagram.