HR6110
HR6110 is a double main-sequence star in the constellation of Corona Borealis.
HR6110 visual magnitude is 6.4. Because of its reltive faintness, HR6110 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 HR6110:
HR6110 is above the horizon from Greenwich, United Kingdom .
Altitude: 35.1°
Azimuth: 279.5°
Direction: West
Celestial coordinates and finder chart of HR6110
HR6110 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 HR6110 are provided in the following table:
The simplified sky map below shows the position of HR6110 in the sky:

Visibility of HR6110 from your location
Location: Greenwich, United Kingdom
Latitude: 51° 28’ 47” N
Longitude: 0° 00’ 00” E
Timezone: Europe/London
Today's HR6110 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 HR6110
The image below is a photograph of HR6110 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 HR6110 is 0.023 arcsec per year in Right Ascension and -0.007 arcsec per year in Declination and the associated displacement for the next 10000 years is represented with the red arrow.

Distance of HR6110 from the Sun and relative movement
HR6110 is distant 515.01 light years from the Sun and it is moving towards the Sun at the speed of 1 kilometers per second.
Spectral properties of HR6110
HR6110 belongs to spectral class A4 and has a luminosity class of V corresponding to a main-sequence star.
The red dot in the diagram below shows where HR6110 is situated in the Hertzsprung–Russell diagram.

HR6110 star system properties
HR6110 is a visual double star which can be observed with binoculars or small telescopes. The table below shows key information about the HR6110 double sysyem: