HR6670 is a sub-giant star in the constellation of Ophiuchus.
HR6670 visual magnitude is 5.77. Because of its reltive faintness, HR6670 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 HR6670:
Celestial coordinates and finder chart of HR6670
HR6670 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 HR6670 are provided in the following table:
The simplified sky map below shows the position of HR6670 in the sky:
Visibility of HR6670 from your location
Digitized Sky Survey image of HR6670
The image below is a photograph of HR6670 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 HR6670 is -0.122 arcsec per year in Right Ascension and 0.069 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR6670 from the Sun and relative movement
HR6670 is distant 102.29 light years from the Sun and it is moving towards the Sun at the speed of 33 kilometers per second.
Spectral properties of HR6670
HR6670 belongs to spectral class F3 and has a luminosity class of IV corresponding to a sub-giant star.
The red dot in the diagram below shows where HR6670 is situated in the Hertzsprung–Russell diagram.