HR4875 is a variable main-sequence star in the constellation of Canes Venatici.
HR4875 visual magnitude is 5.89. Because of its reltive faintness, HR4875 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 HR4875:
Celestial coordinates and finder chart of HR4875
HR4875 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 HR4875 are provided in the following table:
The simplified sky map below shows the position of HR4875 in the sky:
Visibility of HR4875 from your location
Digitized Sky Survey image of HR4875
The image below is a photograph of HR4875 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 HR4875 is -0.097 arcsec per year in Right Ascension and 0.027 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR4875 from the Sun and relative movement
HR4875 is distant 386.71 light years from the Sun and it is moving towards the Sun at the speed of 14 kilometers per second.
Spectral properties of HR4875
HR4875 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 HR4875 is situated in the Hertzsprung–Russell diagram.