HR5035 is a multiple main-sequence star in the constellation of Centaurus.
HR5035 visual magnitude is 4.53. Because of its moderate brightness, HR5035 should be easily visible from locations with dark skyes, while it can be barely visible, or not visible at all, from skyes affected by light pollution.
The table below summarizes the key facts about HR5035:
Celestial coordinates and finder chart of HR5035
HR5035 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 HR5035 are provided in the following table:
The simplified sky map below shows the position of HR5035 in the sky:
Visibility of HR5035 from your location
HR5035 is currently not visible from Greenwich, United Kingdom [change]
Digitized Sky Survey image of HR5035
The image below is a photograph of HR5035 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 HR5035 is -0.039 arcsec per year in Right Ascension and -0.014 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR5035 from the Sun and relative movement
HR5035 is distant 354.35 light years from the Sun and it is moving far from the Sun at the speed of 6 kilometers per second.
Spectral properties of HR5035
HR5035 belongs to spectral class B3 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR5035 is situated in the Hertzsprung–Russell diagram.