υ Coronae Borealis (upsilon Coronae Borealis)

υ Coronae Borealis is a variable and multiple main-sequence star of spectral class A3 in the constellation of Corona Borealis.

υ Coronae Borealis visual magnitude is 5.78. Because of its faintness, υ Coronae Borealis is visible to the naked eye only from locations with very dark skies, while it is not visible at all from skies affected by light pollution.

Celestial Coordinates

Apparent

J2000

Galactic Coordinates

Finder Chart

Magnitude, Color, Spectral Class

The red dot in the diagram below shows where υ Coronae Borealis is situated in the Hertzsprung–Russell diagram.

Star System Properties

υ Coronae Borealis is a visual double star which can be observed with the help of small or medium telescopes. The table below shows key information about the υ Coronae Borealis double sysyem:

Distance, Radial Speed, Proper Motion

υ Coronae Borealis is distant 825.32 light years from the Sun and it is moving far from the Sun at the speed of 7 kilometers per second.

Alternative Designations

Visibility from Your Location

Today's υ Coronae Borealis (upsilon Coronae Borealis) rise, transit and set times from Berala, Australia are the following (all times relative to the local timezone Australia/Sydney):