HR5607 is a multiple giant star in the constellation of Lupus.
HR5607 visual magnitude is 5.15. Because of its reltive faintness, HR5607 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 HR5607:
Celestial coordinates and finder chart of HR5607
HR5607 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 HR5607 are provided in the following table:
The simplified sky map below shows the position of HR5607 in the sky:
Visibility of HR5607 from your location
Digitized Sky Survey image of HR5607
The image below is a photograph of HR5607 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 HR5607 is 0.02 arcsec per year in Right Ascension and -0.003 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR5607 from the Sun and relative movement
HR5607 is distant 367.12 light years from the Sun and it is moving towards the Sun at the speed of 3 kilometers per second.
Spectral properties of HR5607
HR5607 belongs to spectral class G8 and has a luminosity class of III corresponding to a giant star.
The red dot in the diagram below shows where HR5607 is situated in the Hertzsprung–Russell diagram.
HR5607 star system properties
HR5607 is a visual double star which can be observed with binoculars or small telescopes. The table below shows key information about the HR5607 double sysyem: