HR4926 is a multiple main-sequence star in the constellation of Coma Berenices.
HR4926 visual magnitude is 6.2. Because of its reltive faintness, HR4926 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 HR4926:
Celestial coordinates and finder chart of HR4926
HR4926 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 HR4926 are provided in the following table:
The simplified sky map below shows the position of HR4926 in the sky:
Visibility of HR4926 from your location
Digitized Sky Survey image of HR4926
The image below is a photograph of HR4926 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 HR4926 is -0.226 arcsec per year in Right Ascension and 0.06 arcsec per year in Declination and the associated displacement for the next 1000 years is represented with the red arrow.
Distance of HR4926 from the Sun and relative movement
HR4926 is distant 133.12 light years from the Sun and it is moving far from the Sun at the speed of 1 kilometers per second.
Spectral properties of HR4926
HR4926 belongs to spectral class F6 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR4926 is situated in the Hertzsprung–Russell diagram.
HR4926 star system properties
HR4926 is a visual double star which can be observed with binoculars or small telescopes. The table below shows key information about the HR4926 double sysyem: