HR6357 is a sub-giant star in the constellation of Apus.
HR6357 visual magnitude is 6.22. Because of its reltive faintness, HR6357 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 HR6357:
Celestial coordinates and finder chart of HR6357
HR6357 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 HR6357 are provided in the following table:
The simplified sky map below shows the position of HR6357 in the sky:
Visibility of HR6357 from your location
Digitized Sky Survey image of HR6357
The image below is a photograph of HR6357 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 HR6357 is 0.041 arcsec per year in Right Ascension and -0.079 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR6357 from the Sun and relative movement
HR6357 is distant 227.97 light years from the Sun and it is moving towards the Sun at the speed of 24 kilometers per second.
Spectral properties of HR6357
HR6357 belongs to spectral class K1 and has a luminosity class of IV corresponding to a sub-giant star.
The red dot in the diagram below shows where HR6357 is situated in the Hertzsprung–Russell diagram.