HR4537 is a variable main-sequence star in the constellation of Centaurus.
HR4537 visual magnitude is 4.32. Because of its moderate brightness, HR4537 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 HR4537:
Celestial coordinates and finder chart of HR4537
HR4537 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 HR4537 are provided in the following table:
The simplified sky map below shows the position of HR4537 in the sky:
Visibility of HR4537 from your location
HR4537 is currently not visible from Greenwich, United Kingdom [change]
Digitized Sky Survey image of HR4537
The image below is a photograph of HR4537 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 HR4537 is -0.021 arcsec per year in Right Ascension and 0.006 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR4537 from the Sun and relative movement
HR4537 is distant 459.15 light years from the Sun and it is moving far from the Sun at the speed of 29 kilometers per second.
Spectral properties of HR4537
HR4537 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 HR4537 is situated in the Hertzsprung–Russell diagram.