HR4913 is a main-sequence star in the constellation of Centaurus.
HR4913 visual magnitude is 5.16. Because of its reltive faintness, HR4913 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 HR4913:
Celestial coordinates and finder chart of HR4913
HR4913 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 HR4913 are provided in the following table:
The simplified sky map below shows the position of HR4913 in the sky:
Visibility of HR4913 from your location
HR4913 is currently not visible from Greenwich, United Kingdom [change]
Digitized Sky Survey image of HR4913
The image below is a photograph of HR4913 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 HR4913 is -0.026 arcsec per year in Right Ascension and -0.015 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR4913 from the Sun and relative movement
HR4913 is distant 479.41 light years from the Sun and it is moving far from the Sun at the speed of 25 kilometers per second.
Spectral properties of HR4913
HR4913 belongs to spectral class B8 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR4913 is situated in the Hertzsprung–Russell diagram.