HR4619 is a multiple main-sequence star in the constellation of Centaurus.
HR4619 visual magnitude is 6.37. Because of its reltive faintness, HR4619 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 HR4619:
Celestial coordinates and finder chart of HR4619
HR4619 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 HR4619 are provided in the following table:
The simplified sky map below shows the position of HR4619 in the sky:
Visibility of HR4619 from your location
HR4619 is currently not visible from Greenwich, United Kingdom [change]
Digitized Sky Survey image of HR4619
The image below is a photograph of HR4619 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 HR4619 is -0.037 arcsec per year in Right Ascension and 0.002 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Spectral properties of HR4619
HR4619 belongs to spectral class B9 and has a luminosity class of V corresponding to a main-sequence star.
HR4619 star system properties
HR4619 is a visual double star which can be observed with binoculars or small telescopes. The table below shows key information about the HR4619 double sysyem: