HR4719
HR4719 is a multiple main-sequence star in the constellation of Coma Berenices.
HR4719 visual magnitude is 6.42. Because of its reltive faintness, HR4719 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 HR4719:
Celestial coordinates and finder chart of HR4719
HR4719 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 HR4719 are provided in the following table:
The simplified sky map below shows the position of HR4719 in the sky:

Visibility of HR4719 from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Timezone: Europe/London
Today's HR4719 rise, transit and set times from Greenwich, United Kingdom are the following (all times relative to the local timezone Europe/London):
Digitized Sky Survey image of HR4719
The image below is a photograph of HR4719 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 HR4719 is -0.014 arcsec per year in Right Ascension and -0.004 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.

Distance of HR4719 from the Sun and relative movement
HR4719 is distant 318.67 light years from the Sun and it is moving towards the Sun at the speed of 6 kilometers per second.
Spectral properties of HR4719
HR4719 belongs to spectral class A7 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR4719 is situated in the HertzsprungāRussell diagram.

HR4719 star system properties
HR4719 is a visual double star which can be observed with the help of large telescopes. The table below shows key information about the HR4719 double sysyem: