HR4590 is a main-sequence star in the constellation of Corvus.
HR4590 visual magnitude is 5.26. Because of its reltive faintness, HR4590 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 HR4590:
Celestial coordinates and finder chart of HR4590
HR4590 is situated close to the celestial equator, as such, it is at least partly visible from both hemispheres in certain times of the year. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR4590 are provided in the following table:
The simplified sky map below shows the position of HR4590 in the sky:
Visibility of HR4590 from your location
Digitized Sky Survey image of HR4590
The image below is a photograph of HR4590 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 HR4590 is -0.021 arcsec per year in Right Ascension and 0.013 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR4590 from the Sun and relative movement
HR4590 is distant 1,752.69 light years from the Sun and it is moving far from the Sun at the speed of 2 kilometers per second.
Spectral properties of HR4590
HR4590 belongs to spectral class B1 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR4590 is situated in the Hertzsprung–Russell diagram.