HR5413 is a double main-sequence star in the constellation of Lupus.
HR5413 visual magnitude is 5.37. Because of its reltive faintness, HR5413 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 HR5413:
Celestial coordinates and finder chart of HR5413
HR5413 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 HR5413 are provided in the following table:
The simplified sky map below shows the position of HR5413 in the sky:
Visibility of HR5413 from your location
HR5413 is currently not visible from Greenwich, United Kingdom [change]
Digitized Sky Survey image of HR5413
The image below is a photograph of HR5413 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 HR5413 is -0.052 arcsec per year in Right Ascension and -0.047 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR5413 from the Sun and relative movement
HR5413 is distant 222.37 light years from the Sun
Spectral properties of HR5413
HR5413 belongs to spectral class A1 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR5413 is situated in the Hertzsprung–Russell diagram.
HR5413 star system properties
HR5413 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 HR5413 double sysyem: