HR5327

HR5327 is a main-sequence star in the constellation of Apus.

HR5327 visual magnitude is 6.42. Because of its reltive faintness, HR5327 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 HR5327:

Celestial coordinates and finder chart of HR5327

HR5327 is situated close to the southern celestial pole and, as such, it is easilty visible for most part of the year from the southern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR5327 are provided in the following table:

The simplified sky map below shows the position of HR5327 in the sky:

Visibility of HR5327 from your location

HR5327 is currently not visible from Greenwich, United Kingdom edit_location_alt

Digitized Sky Survey image of HR5327

The image below is a photograph of HR5327 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 HR5327 is 0.001 arcsec per year in Right Ascension and -0.019 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.

Distance of HR5327 from the Sun and relative movement

HR5327 is distant 881.08 light years from the Sun and it is moving far from the Sun at the speed of 27 kilometers per second.

Spectral properties of HR5327

HR5327 belongs to spectral class B8 and has a luminosity class of V corresponding to a main-sequence star.

The red dot in the diagram below shows where HR5327 is situated in the Hertzsprung–Russell diagram.

Alternative designations of HR5327