HR538 is a main-sequence star in the constellation of Perseus.
HR538 visual magnitude is 6.26. Because of its reltive faintness, HR538 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 HR538:
Celestial coordinates and finder chart of HR538
HR538 is situated north of the celestial equator, as such, it is more easily visible from the northern hemisphere. Celestial coordinates for the J2000 equinox as well as galactic coordinates of HR538 are provided in the following table:
The simplified sky map below shows the position of HR538 in the sky:
Visibility of HR538 from your location
HR538 is circumpolar and transits at 01:59 UTC (altitude: 90.0°)
Digitized Sky Survey image of HR538
The image below is a photograph of HR538 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 HR538 is -0.011 arcsec per year in Right Ascension and -0.009 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.
Distance of HR538 from the Sun and relative movement
HR538 is distant 494.69 light years from the Sun and it is moving far from the Sun at the speed of 6 kilometers per second.
Spectral properties of HR538
HR538 belongs to spectral class A3 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR538 is situated in the Hertzsprung–Russell diagram.