HR6627 is a double main-sequence star in the constellation of Hercules.
HR6627 visual magnitude is 5.72. Because of its reltive faintness, HR6627 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 HR6627:
Celestial coordinates and finder chart of HR6627
HR6627 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 HR6627 are provided in the following table:
The simplified sky map below shows the position of HR6627 in the sky:
Visibility of HR6627 from your location
Digitized Sky Survey image of HR6627
The image below is a photograph of HR6627 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 HR6627 is 0.011 arcsec per year in Right Ascension and -0.007 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR6627 from the Sun and relative movement
HR6627 is distant 367.95 light years from the Sun and it is moving far from the Sun at the speed of 3 kilometers per second.
Spectral properties of HR6627
HR6627 belongs to spectral class A1 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR6627 is situated in the Hertzsprung–Russell diagram.
HR6627 star system properties
HR6627 is a visual double star which can be observed with the help of large telescopes. The table below shows key information about the HR6627 double sysyem: