HR5637 is a double supergiant star in the constellation of Lupus.
HR5637 visual magnitude is 5.54. Because of its reltive faintness, HR5637 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 HR5637:
Celestial coordinates and finder chart of HR5637
HR5637 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 HR5637 are provided in the following table:
The simplified sky map below shows the position of HR5637 in the sky:
Visibility of HR5637 from your location
Digitized Sky Survey image of HR5637
The image below is a photograph of HR5637 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 HR5637 is -0.002 arcsec per year in Right Ascension and -0.008 arcsec per year in Declination and the associated displacement for the next 100000 years is represented with the red arrow.
Distance of HR5637 from the Sun and relative movement
HR5637 is distant 2,024.84 light years from the Sun and it is moving towards the Sun at the speed of 4 kilometers per second.
Spectral properties of HR5637
HR5637 belongs to spectral class G2 and has a luminosity class of I corresponding to a supergiant star.
The red dot in the diagram below shows where HR5637 is situated in the Hertzsprung–Russell diagram.
HR5637 star system properties
HR5637 is a visual double star which can be observed only with the help of very large telescopes. The table below shows key information about the HR5637 double sysyem: