HR5625 is a main-sequence star in the constellation of Lupus.
HR5625 visual magnitude is 5.85. Because of its reltive faintness, HR5625 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 HR5625:
Celestial coordinates and finder chart of HR5625
HR5625 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 HR5625 are provided in the following table:
The simplified sky map below shows the position of HR5625 in the sky:
Visibility of HR5625 from your location
Digitized Sky Survey image of HR5625
The image below is a photograph of HR5625 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 HR5625 is -0.027 arcsec per year in Right Ascension and -0.018 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR5625 from the Sun and relative movement
HR5625 is distant 444.14 light years from the Sun and it is moving far from the Sun at the speed of 1 kilometers per second.
Spectral properties of HR5625
HR5625 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 HR5625 is situated in the Hertzsprung–Russell diagram.