HR5357 is a main-sequence star in the constellation of Centaurus.
HR5357 visual magnitude is 5.94. Because of its reltive faintness, HR5357 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 HR5357:
Celestial coordinates and finder chart of HR5357
HR5357 is situated south of the celestial equator, as such, it is more easily visible from the southern emisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR5357 are provided in the following table:
The simplified sky map below shows the position of HR5357 in the sky:
Visibility of HR5357 from your location
Digitized Sky Survey image of HR5357
The image below is a photograph of HR5357 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 HR5357 is -0.047 arcsec per year in Right Ascension and -0.059 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR5357 from the Sun and relative movement
HR5357 is distant 223.29 light years from the Sun
Spectral properties of HR5357
HR5357 belongs to spectral class A2 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR5357 is situated in the Hertzsprung–Russell diagram.