HR6875

HR6875 is a variable and double main-sequence star in the constellation of Corona Australis.

HR6875 visual magnitude is 5.25. Because of its reltive faintness, HR6875 should be visible only from locations with dark skies, while it is not visible at all from skies affected by light pollution.

The proper motion of HR6875 is -0.002 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.

Key facts about HR6875

Celestial coordinates and finder chart of HR6875

HR6875 is situated south of the celestial equator, as such, it is more easily visible from the southern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR6875 are provided in the following table:

The simplified sky map below shows the position of HR6875 in the sky:

Visibility of HR6875 from your location

HR6875 is currently not visible from Greenwich, United Kingdom edit_location_alt

Distance of HR6875 from the Sun and relative movement

HR6875 is distant 524.12 light years from the Sun

Spectral properties of HR6875

HR6875 belongs to spectral class B2 and has a luminosity class of V corresponding to a main-sequence star.

The red dot in the diagram below shows where HR6875 is situated in the Hertzsprung–Russell diagram.

HR6875 star system properties

HR6875 is a visual double star which can be observed with the help of small or medium telescopes. The table below shows key information about the HR6875 double sysyem:

Alternative designations of HR6875