HR5687 is a variable main-sequence star in the constellation of Lupus.
HR5687 visual magnitude is 5.59. Because of its reltive faintness, HR5687 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 HR5687:
Celestial coordinates and finder chart of HR5687
HR5687 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 HR5687 are provided in the following table:
The simplified sky map below shows the position of HR5687 in the sky:
Visibility of HR5687 from your location
Digitized Sky Survey image of HR5687
The image below is a photograph of HR5687 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 HR5687 is -0.014 arcsec per year in Right Ascension and -0.024 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR5687 from the Sun and relative movement
HR5687 is distant 514.20 light years from the Sun and it is moving far from the Sun at the speed of 11 kilometers per second.
Spectral properties of HR5687
HR5687 belongs to spectral class B7 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR5687 is situated in the Hertzsprung–Russell diagram.